The galaxy presents as a primarily smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a yellowish hue, potentially indicating a population of older stars. Moving outward from the core, a gradual transition to a bluer color is observed, suggesting the presence of younger, hotter stars in the outer regions. There appears to be little to no spiral arm structure discernible in the image. The overall shape approximates a circular form, with a slight elongation noticeable. No significant signs of tidal disturbances or ongoing major merging events are immediately evident, though subtle asymmetries cannot be ruled out at this resolution.
