The galaxy presents as a relatively smooth, elliptical-like object with a slightly elongated morphology. It appears to have a concentrated central bulge that gradually fades into a less defined halo. The color profile suggests a population dominated by older stars, as indicated by the yellowish-red hue. There is little to no visible evidence of distinct spiral arm structures or significant dust lanes. The overall structure shows no signs of major ongoing mergers or tidal disruptions, though some minor asymmetry cannot be ruled out entirely.
