The galaxy presents as a relatively smooth, elliptical-like structure. The light is centrally concentrated, appearing most luminous towards the core, with a gradual decrease in intensity outwards. It's generally round, with no apparent strong distortions or tidal features suggesting recent major merger activity. The galaxy exhibits a yellowish-white hue in the central region, possibly indicating an older stellar population or a larger proportion of stars in the redder part of the spectrum, and there is some suggestion of faint bluer light on the outer edges of the object. There are no obvious spiral arm features, bright star-forming regions, or a prominent disk component. The lack of distinct features supports its classification as likely elliptical in morphology.
