The galaxy appears to be a relatively smooth, elliptical galaxy with a noticeable color gradient. The central region exhibits a pronounced orange hue, suggesting a concentration of older stellar populations. This core transitions to a greenish-yellow outer region, which could indicate the presence of younger stars or regions of active star formation, though this is subtle. The galaxy's overall shape is somewhat elongated, falling between a perfect circle and a cigar shape, indicating a moderate degree of ellipticity. There is no strong visual evidence of major disturbances due to recent mergers. There appears to be a slight asymmetry in the outer regions, but no clear tidal tails or other indicators of an ongoing interaction.