The galaxy presents as a largely smooth, elliptical structure with a concentrated, bright central bulge. The luminosity appears to diminish gradually from the core outwards. The overall color index suggests a population of older stars dominating the light output, likely with lower ongoing star formation. The galaxy exhibits a nearly round morphology, with only minor deviations from a perfect circular shape. There's no obvious evidence of spiral arms, a distinct disk, or significant tidal disturbances indicative of recent major mergers, though there is a slight asymmetry that could suggest a minor interaction. The absence of strong blue or ultraviolet light further supports a classification as a galaxy with a passively evolving stellar population.
