The galaxy presents as a luminous, elliptical morphology. It exhibits a generally smooth appearance, with little discernible internal structure or arm features. The light distribution is concentrated towards the center, indicating a significant bulge component. The color index appears relatively red, suggesting an older stellar population and a lack of ongoing, significant star formation. There are indications of potential minor disturbances in the galaxy's structure, however, more detailed investigation is needed. The overall appearance does not strongly suggest a major ongoing merger event. The galaxy's shape is not perfectly circular, exhibiting a moderate degree of ellipticity.
