The galaxy presents as a slightly elliptical, primarily smooth structure with a noticeable central bulge. Its overall color leans toward a warm, yellow-orange hue, suggesting an older stellar population and reduced recent star formation. The galaxy exhibits a gradual decrease in surface brightness from the core outwards, and appears to have little discernible spiral arm structure. It is primarily of intermediate roundness, lacking a clear disk or bar feature. The galaxy is likely undergoing only weak merging processes, if any.
