The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a yellowish hue, suggesting an older stellar population with lower levels of ongoing star formation. The galaxy displays a generally rounded shape with no apparent disk structure or spiral arms. There are no obvious signs of major mergers or significant tidal disturbances in its morphology. The light distribution indicates a relatively even profile, without strong, distinct features. Overall, this galaxy likely represents a mature system with minimal recent star-forming activity and a relatively high degree of symmetry.
