This galaxy appears as a concentrated central bulge surrounded by a diffuse halo. The central region exhibits a yellowish-orange hue, suggesting a population of older stars. The overall shape is nearly circular, with a relatively smooth appearance and no immediately obvious spiral arm structures or prominent dust lanes. The faint, extended halo seems to gradually fade into the background, suggesting a decreasing stellar density further from the galactic center. There is no apparent evidence of any ongoing major mergers or tidal disturbances in the image.
