The galaxy presents a generally smooth and elliptical morphology. A bright, concentrated central bulge dominates the overall structure, exhibiting a yellowish-white hue indicative of an older stellar population. Moving outward from the core, the light gradually diminishes, with a faint, diffuse halo extending beyond the main body. A subtle bluing is visible in the outer regions, suggesting the presence of younger, hotter stars at the periphery, even though the galaxy is, on average, more evolved. There is a hint of a disk-like structure, but it is faint and not particularly well-defined. No significant tidal features or signs of a major ongoing merger are immediately apparent. There is some minor disturbance in the outer disc. The object appears to be relatively isolated and undisturbed. The galaxy does not exhibit any pronounced dust lanes or spiral arms, pointing to a lack of ongoing active star formation within the central regions, although there may be star formation occurring at the outer edges. Overall, the galaxy appears to be a fairly massive, early-type system.
