The galaxy presents a generally smooth, elliptical morphology. It appears moderately compact with a fairly concentrated central bulge. The overall color profile suggests the presence of both older stellar populations and some ongoing star formation, with the central region exhibiting a slightly yellower hue and the outer regions a bluer hue. There is no obvious indication of spiral arms or a well-defined disk structure. There is a slight indication of tidal interactions or minor disturbance; however, it remains largely undisturbed.
