The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, but it is not perfectly spherical, exhibiting a slightly elongated shape. A bright central bulge dominates the light profile, transitioning smoothly into a fainter, diffuse halo. There are no prominent spiral arms or distinct dust lanes visible. Faint blue hues are subtly present within the outer regions, suggesting the possibility of ongoing, though limited, star formation. There are some small disturbances possibly suggestive of a minor interaction or merging event. Overall, it is a quiescent galaxy, likely dominated by an older stellar population.
