The galaxy presents as a single, moderately luminous object with a dominant central bulge. The morphology appears largely smooth, lacking well-defined spiral arms or distinct features. The galaxy is approximately elliptical in shape, displaying a slight elongation. A faint, diffuse halo surrounds the brighter central region, suggesting the presence of older stellar populations extending beyond the main body. There is no strong evidence of ongoing major mergers or tidal disturbances in this image, though subtle irregularities in the outer halo cannot be ruled out without deeper observations. The overall color profile indicates the galaxy has a population of older stars, with only a small level of ongoing star formation activity.
