The galaxy presents an overall smooth appearance, suggesting a relatively evolved system. It exhibits a largely elliptical morphology, appearing quite round. There is some evidence of potential tidal features or minor disturbances in the overall structure, and there is an indication of ongoing or recent merger activity. The galaxy displays a central concentration of light that appears yellow, with more red coloration in the outer regions, which could indicate a central bulge population of older stars and on-going star formation, or dust, in the outer regions. There is an apparent interaction or overlap with another, dimmer object. There are signs of faint extended emission beyond the main body of the galaxy, potentially indicating a halo or tidal debris.
