The galaxy presents as an elliptical morphology, exhibiting a relatively smooth and concentrated light distribution. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The color profile suggests a population of older stars, leaning towards redder hues. There is a slight elongation but the object is primarily round. A notable fraction of the image appears to indicate a merger, possibly an ongoing interaction or recent coalescence with another galactic structure based on a minor distortion. There seems to be minimal evidence of active star formation within the galaxy, with a lack of bright blue regions typically associated with young, massive stars. The overall appearance indicates a evolved and quiescent stellar population.
