The galaxy exhibits a relatively compact morphology, appearing nearly elliptical in projection. A bright central core dominates the galaxy's luminosity profile, suggesting a significant concentration of stars or potentially an active galactic nucleus.

The main body of the galaxy appears relatively smooth, with a noticeable lack of strong spiral arm structures or prominent dust lanes. Some faint, diffuse features appear to extend away from the central region, suggesting the presence of a weak tidal tail or stellar stream. These features are more apparent on one side of the galaxy than the other, and have a slight reddish tint compared to the main body of the galaxy.

The overall color of the galaxy is moderately blue, indicating the presence of a young stellar population, though not overwhelmingly so. This implies a moderate level of ongoing star formation within the galaxy. The degree of color variation across the galaxy is limited, suggesting a somewhat uniform stellar population distribution, excluding the redder feature on the right side of the galaxy.
