The galaxy presents as a slightly elongated, concentrated source of light. The overall color is yellowish-orange, suggestive of an older stellar population. The light distribution is smooth, without any visually distinct spiral arms or prominent dust lanes. The shape tends toward being elliptical, possibly an elliptical galaxy. There are very faint hints of asymmetry or a slight extension on one side, suggesting possible minor tidal disturbance or interaction, though this is not a distinct merger event. There is no pronounced nucleus or other significant internal structure discernible at this resolution.
