This galaxy presents as a relatively small, elliptical-like structure. A bright, concentrated core dominates the galaxy's center, exhibiting a roughly symmetrical distribution of light intensity. The overall color profile suggests a population of older stars, indicated by the slightly redder hues present outside of the core. 

Evidence of possible disturbances or tidal features is subtle, but the slight asymmetry in the outer regions and the fuzzy edges may indicate minor gravitational interactions with another galaxy or past merger events. There is no clear indication of prominent spiral arms or a well-defined disk. A somewhat smooth morphology is suggested, and a significant amount of light is emanating from the central region.
