The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates the luminosity profile. This central region exhibits a yellowish-orange color, suggesting a population of older stars. Extending outward from the bulge is a faint, diffuse halo. This outer region is somewhat more blue, which could be interpreted as the presence of younger stellar populations. No prominent spiral arm structures are visible. The galaxy's overall roundness indicates a classification trending toward E0-E3 on the Hubble sequence. There is no evidence of major mergers or significant tidal disturbances. The galaxy appears undisturbed, suggesting it is not undergoing a major interaction. There may be a small degree of minor disturbance or faint features in the outskirts, warranting closer investigation.
