The galaxy exhibits a morphology that appears largely smooth and elliptical in nature. A significant portion of its light is concentrated in a central bulge, suggesting a high degree of stellar density within this region. This central region appears to be nearly circular, rather than elongated. There is an apparent tidal tail or streamer extending outward from one side of the main galactic body. The tail is faint and diffuse, indicating a possible interaction or past merger event. The galaxy's color indices suggest it is composed mostly of older, redder stars. Star formation appears to be low within the galaxy itself. The galaxy displays a high degree of overall symmetry.
