The galaxy appears as a roughly elliptical, unresolved object. A bright central bulge dominates the structure, with a gradual decrease in luminosity moving outward. The galaxy exhibits a smooth overall appearance, with no readily discernible spiral arms or significant dust lanes visible in this image. There are hints of an extended, diffuse halo surrounding the central region, characterized by a faint, indistinct glow. The color profile suggests a population of older stars, as indicated by the redder hue, particularly in the outer regions. There is no obvious evidence of ongoing major merger events. Slight asymmetry and subtle perturbations can be observed, possibly indicating a minor interaction or internal dynamic processes. The apparent size of the object is relatively small, suggesting moderate physical dimensions at its distance.
