The galaxy presents a generally smooth, elliptical morphology. A concentrated, bright central bulge is apparent, exhibiting a yellowish hue, likely indicative of an older stellar population. Fainter, bluish-tinted light extends outwards from the central region in a flattened, disk-like structure. This suggests the presence of some ongoing star formation, albeit relatively subdued. The overall shape leans towards a slightly elongated or oval form rather than being perfectly spherical. There appears to be some minor gravitational disturbance or interaction, though its effect on the galaxy's main structure seems minimal.
