The galaxy exhibits a primarily smooth morphology, with a discernible elliptical shape. The light distribution appears relatively even across its body, suggesting a lack of distinct spiral arms or prominent features. The overall color is yellowish-white, indicating a potential older stellar population.

Evidence suggests the galaxy may be undergoing or has undergone a merger event, with some minor distortions or irregularities visible in its outer regions. These could also be tidal tails or remnants of past interactions with another galaxy. There appears to be some disturbance in the smoothness. Some minor disturbances may be responsible for the distortion.
