The galaxy presents a largely smooth, elliptical morphology, exhibiting a generally round shape. The central bulge region appears to dominate the overall luminosity, displaying a yellowish hue, suggestive of an older stellar population. There is evidence of possible tidal interaction or an ongoing merger event. A secondary, smaller, and slightly bluer component is observed adjacent to the primary body, indicative of possible star formation activity spurred by the gravitational interaction. The overall structure suggests a system that is either in the late stages of a merger or experiencing a minor disturbance. The galaxy has an apparent moderate magnitude.
