The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, with a ratio of major to minor axis suggesting it is neither perfectly spherical nor highly elongated. There are no obvious spiral arms or distinct bar structures visible in this image, implying a lack of significant organized disk structure. The color appears relatively uniform across the galaxy, with a slightly yellow hue indicative of a population of older stars and possibly some dust obscuration. There is no visual evidence of ongoing major mergers or tidal disturbances.
