The galaxy presents as a relatively smooth and rounded object. It exhibits a centrally concentrated luminosity profile, with light intensity decreasing gradually outward from the core. The galaxy appears to be slightly elliptical in shape, with a subtle elongation. There is no obvious spiral arm structure or dust lane obscuration visible. The color appears to be consistent with an older stellar population, suggesting a relatively quiescent star formation history. The overall morphology suggests a possible elliptical galaxy classification.
