The galaxy presents as a relatively smooth, centrally concentrated object with a slight overall elliptical shape. Its core region is significantly brighter and exhibits a yellowish-white hue, suggesting a population of older stars. Extending outward from this core is a fainter, reddish-tinged disk or halo, potentially indicating a distribution of cooler stars or dust. The disk appears mostly featureless, with no obvious spiral arm structure or distinct dust lanes visible. The galaxy exhibits a degree of asymmetry, where one side of the disk appears slightly more extended than the other. There's a hint of possible tidal interactions or minor disturbances to the morphology.
