The galaxy presents as a relatively smooth, centrally concentrated object. There is a clear radial gradient in luminosity, peaking at a bright, well-defined core, and gradually decreasing outwards to a fainter, less distinct halo. The overall shape appears roughly elliptical, tending toward a more rounded, rather than elongated, form. No distinct spiral arm structures or prominent dust lanes are discernible within the resolution of the image. There are hints of possible minor disturbances or irregularities in the outer regions, but no definitive evidence of major mergers or tidal interactions. The color profile suggests a population dominated by older stars, with a yellow-red hue. The estimated size of the galaxy is rather compact.
