The galaxy presents a predominantly elliptical morphology, appearing as a flattened spheroid. It exhibits a distinct central bulge that is bright and concentrated. A fainter, more diffuse halo extends outwards from this central region, showing a noticeable elongation. This galaxy's overall color is observed as a slightly reddish hue, particularly in the outer regions, possibly indicating an older stellar population. In the center of the galaxy, there is a region of bluer light which is possibly caused by active star formation. Some subtle asymmetrical features appear to be present on one side of the galaxy, potentially suggesting a minor interaction or tidal disturbance. These features are faint but could be indicative of ongoing dynamical processes. Overall, the galaxy appears to be a relatively isolated system.