The galaxy presents as a generally smooth and rounded object with a concentrated central bulge. The color distribution is primarily yellow-white, suggesting an older stellar population dominating the light output. There is little evidence of prominent spiral arm structures or significant dust lanes. A subtle color gradient can be observed, with the central region appearing slightly more yellow compared to the surrounding area. The outer edges of the galaxy fade gradually into the background, indicating a diffuse halo or extended stellar component. There are no obvious signs of recent major merger activity or strong tidal disturbances, with the galaxy displaying a relatively undisturbed morphology. Faint, diffuse features may be present in the outer regions, warranting further investigation to determine if they are associated with minor interactions.