The galaxy presents as a structured system, seemingly composed of two distinct components. The primary body exhibits a smooth, elliptical morphology, with a concentrated central bulge that transitions into a more diffuse halo. The color profile suggests an older stellar population, dominated by redder wavelengths. Evident is a secondary, smaller component situated nearby. The overall structure suggests a possible ongoing interaction or merger event, where a smaller galaxy is in the process of being accreted by a larger one. Evident tidal distortions or disruptions in either galaxy are absent, indicating a well-advanced stage of merger. Star formation is either quiescent or occurring at a very low rate.