The galaxy appears to be elliptical in shape. The central region exhibits a high concentration of light, appearing yellow-orange in color, suggesting an older stellar population dominating the core. Moving outwards from the core, the galaxy exhibits a diffuse, less luminous region. The outer regions show a slight hint of blue light, suggestive of the presence of a younger, albeit limited, stellar population. There is no apparent disk structure or spiral arm features visible. The galaxy exhibits a relatively smooth overall morphology, with no obvious signs of major mergers or significant tidal disturbances. Slight asymmetry may be present in the outer regions.
