This galaxy exhibits a generally smooth morphology, with a notable concentration of light towards the galactic center, suggesting the presence of a bulge. The galaxy appears to be elliptical in shape, though it's not perfectly round. The light distribution extends outwards from the center, gradually decreasing in intensity. There is a subtle blue tint, more prominent in the outer regions, which could indicate the presence of a younger stellar population or ongoing star formation, albeit at a low rate. No distinct spiral arms or bars are visible, further supporting its classification as an elliptical galaxy. There is no evidence of any major merging activity or significant tidal disturbances in its immediate vicinity.
