The galaxy exhibits a centrally concentrated luminosity profile, appearing as a single, largely unresolved luminous object. A gradual decrease in surface brightness extends outward from the bright core. The overall form suggests a possible elliptical morphology, lacking discernible spiral arms or a distinct disk structure. The galaxy's color appears predominantly yellowish-white. There is a smaller, dimmer object close to the bottom side of the galaxy, potentially due to some sort of interaction. It is not clear if this is a foreground or background object. No clear dust lanes or other prominent features indicative of active star formation are apparent. The observed characteristics point toward a relatively evolved system, potentially an elliptical galaxy with an older stellar population. There is potentially an area of disturbance near the center. There is no evidence of a strong tidal tail or merging interaction.
