The galaxy presents a smooth, rounded morphology, indicative of an elliptical galaxy. The light distribution is centrally concentrated, with a gradual decline in intensity moving outwards. The color profile appears relatively uniform across the galaxy, suggesting a consistent stellar population likely dominated by older, redder stars. There is no discernible disk structure or spiral arms. The axial ratio suggests the galaxy is nearly circular in projection, with a slight ellipticity. No obvious signs of ongoing mergers or tidal disturbances are apparent in the image.
