The galaxy presents as a centrally concentrated system with a generally smooth appearance. Its morphology is primarily elliptical, though it does exhibit a slight deviation from perfect circularity, appearing somewhat elongated. The light distribution is relatively even, with a noticeable central bulge that radiates outwards. There's evidence of a subtle disk component contributing to its overall structure.  The color profile suggests a stellar population of intermediate age, with some indication of ongoing, albeit moderate, star formation. There are possible signs of minor disturbances in the outer regions. The galaxy appears relatively isolated, showing no obvious signs of interaction or merging with other significant systems.
