The galaxy appears as a relatively smooth, elliptical-shaped object. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. The galaxy's light profile gradually diminishes from the center outwards, displaying a diffuse halo that extends moderately in all directions. There is a slight elongation, indicating it might not be perfectly spherical. The color is generally yellowish, with some areas of red, possibly indicative of an older stellar population. There are no clearly defined spiral arms or prominent dust lanes visible, further supporting its classification as an elliptical galaxy. Based on the slight disturbances of the galaxy, there does not appear to be major disruptions due to merging activity or interactions.
