The galaxy exhibits an elliptical morphology, appearing as a smooth, concentrated spheroid of light. The central region is brighter and more densely packed than the outer regions, with a gradual decrease in luminosity towards the periphery. The galaxy displays a moderate ellipticity, deviating somewhat from a perfectly circular shape and tending toward a cigar-like shape. There is no visible dust lane, spiral arm structure, or significant star-forming regions. The overall color is slightly redder in the central regions, suggesting an older stellar population. No major mergers or tidal disturbances are observed, but a slight asymmetry or minor disturbance may be present in the outer regions.
