The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes. The light profile appears centrally concentrated and gradually fades outward, indicating a relatively old stellar population. The galaxy exhibits a yellowish-red hue, consistent with evolved stars and a lower rate of ongoing star formation. There's a slight elongation in shape, suggesting a deviation from perfect sphericity, but it appears largely undisturbed with no obvious signs of recent major mergers or tidal interactions. The overall impression is that of a quiescent galaxy, likely dominated by older stars.
