The galaxy presents a generally smooth, elliptical morphology. There is a slight elongation to its shape, deviating somewhat from a perfect circle. The light distribution within the galaxy appears relatively uniform, with a subtle concentration towards the center. There is evidence of a possible minor disturbance in the overall structure, although the features are not highly pronounced. The galaxy displays a yellow/orange color, suggestive of an older stellar population. This is consistent with low ongoing star formation activity. There is no clear presence of spiral arms or a well-defined disk. The galaxy's relatively compact appearance indicates a high mass concentration within a small radius.