The galaxy presents as an elliptical morphology, appearing generally smooth with a high degree of central concentration. It is characterized by a slightly elongated, though primarily rounded, shape. The color profile exhibits a gradient, with the core region displaying a brighter, bluer hue that fades into a redder, more diffuse halo. There is no apparent spiral structure or significant dust lane visible in this image. The object does not display any signs of a major ongoing merger, or tidal disturbances, but there could be minor disturbances. The estimated size is relatively small, indicating it is either a dwarf galaxy or is very distant. Based on the blue core and implied star formation rate, it is probable the galaxy's star formation rate is rather low.
