The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its light profile shows a distinct radial gradient, with the core exhibiting a brighter, more yellowish hue, suggesting a population of older stars and/or a significant dust component. The outer regions of the galaxy fade gradually into the background sky, displaying a redder color than the core. There is no visually apparent disk structure or spiral arms. The overall symmetry and lack of any obvious tidal features suggest that it is not currently undergoing a major merger event, although minor disturbances cannot be ruled out at this resolution. The galaxy displays a fairly compact size.
