The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, exhibiting a moderate degree of ellipticity without a pronounced disk structure. The central bulge is prominent and displays a yellowish hue, suggesting an older stellar population with minimal ongoing star formation. The outer regions of the galaxy gradually fade into the background, indicating a lack of distinct, sharp edges or spiral arms. No obvious signs of major mergers or tidal disturbances are apparent; instead, the structure appears relaxed and evolved. The overall color profile indicates that any recent or current star formation activity is likely subdued.
