The galaxy appears as a relatively compact object. It exhibits a smooth, elliptical morphology, with no readily discernible spiral arm structures or bar features. The light distribution indicates a centrally concentrated luminosity profile. The color is generally consistent with a population of older stars, exhibiting a redder hue, though there is a suggestion of some bluer light emanating from its core. There is no obvious evidence of any major ongoing mergers or significant tidal disturbances in this image, though there might be some minor distortion.
