The galaxy appears to be a relatively compact object, exhibiting a smooth, elliptical morphology. The color profile suggests a dominant population of older stars, indicated by its redder hue. No distinct spiral arms or prominent dust lanes are discernible, supporting its classification as an elliptical galaxy. There is a slight asymmetry in the light distribution, potentially indicating a minor interaction or disturbance, though the overall structure appears largely undisturbed. The galaxy seems to be relatively isolated, with no other large galaxies nearby that could be causing tidal effects, however there appears to be a small satellite galaxy nearby.
