The galaxy presents as a relatively smooth object with a concentrated central region. Its overall form appears to be elliptical, though not perfectly spherical. There is a slight elongation, suggesting it may be an elliptical galaxy with some level of flattening.

A color gradient is visible. The central bulge exhibits a yellowish-red hue, indicating a population of older stars. The outer regions have a bluer tint, potentially hinting at ongoing star formation. No distinct spiral arm structures are discernible.

There may be some signs of minor disturbances, but no major signs of any merging events. Overall, this galaxy appears to be in a relatively settled state, consistent with an elliptical galaxy that is not actively undergoing significant interactions.
