The galaxy presents a relatively smooth, elliptical morphology. There is an apparent lack of distinct spiral arms or a prominent disk structure. The central region exhibits a bright, concentrated bulge, suggestive of a high stellar density. The galaxy's color profile appears generally redder, potentially indicating an older stellar population and lower ongoing star formation activity. Faint, extended light is observed around the central region, possibly indicating a diffuse halo or tidal features, though further investigation is needed to confirm this. There is no obvious evidence of a major merger event or significant tidal disturbances. The galaxy exhibits a slightly elongated, but generally rounded shape. 
