The galaxy presents as a singular, moderately compact object. The overall form appears largely spheroidal with a high degree of central concentration. The core exhibits a strong, relatively uniform luminosity, suggesting a significant population of older stars.

There is a clear asymmetry in the light distribution, with a noticeable extension or tidal feature emanating from the main body of the galaxy to the lower left. This extension displays a redder hue compared to the central core. The asymmetry could be indicative of a minor tidal interaction or past merger event. Evidence of more prominent spiral arm structures or a well-defined disk component is absent, which supports an elliptical classification, or perhaps a lenticular galaxy with a poorly defined disk. Based on color, there may be a small amount of ongoing star formation.

The absence of fine-grained morphological features suggests a relatively relaxed system, although the single feature on one side hints that it may be only partially relaxed from previous interactions. The galaxy displays an intermediate level of luminosity. Overall, the characteristics suggest a mid-mass galaxy at intermediate redshift.
