The galaxy presents an elliptical morphology, appearing largely spheroidal and relatively smooth in texture. A bright, concentrated central bulge dominates the structure, with a gradual decrease in luminosity extending outwards. The color profile indicates a yellow-orange hue concentrated within the core, potentially signifying an older stellar population. Fainter, bluish halos surround the core, possibly representing a population of younger stars in the outer regions. Slight asymmetries are visible, suggestive of minor gravitational interactions or internal dynamics. The overall light distribution and color suggest a relatively mature galaxy with ongoing, but not particularly vigorous, star formation.
