The galaxy presents a generally smooth and elliptical morphology. A concentrated central bulge is visible, emitting a significant amount of light. There is a subtle color gradient, appearing slightly bluer in the central region, possibly indicating a small amount of recent or ongoing star formation within the core. The outer regions of the galaxy appear redder, suggesting an older stellar population is dominant in those areas. No distinct spiral arms or bar structures are discernible within the image. There are slight asymmetries in the outer halo but no strong evidence for any major mergers or tidal disturbances. Overall, the galaxy presents a regular and relatively undisturbed structure.
