The galaxy presents a generally smooth, elliptical morphology, lacking prominent spiral arm structures. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue indicative of an older stellar population. Moving outwards from the core, a more diffuse halo is observed with a bluer tint, suggesting the presence of younger, hotter stars in the outer regions. The overall shape is somewhat rounded, with only a slight elongation visible. There is some visual evidence suggesting minor gravitational interaction or disturbance, possibly an ongoing or past minor merger event. However, the galaxy's structure is primarily undisturbed.
