The galaxy appears as a slightly elongated, diffuse object with a noticeable central bulge. The light distribution suggests a higher concentration of older stars in the central region, grading into a more diffuse halo. The overall color is reddish-yellow, indicating a relatively evolved stellar population. There is no clear evidence of spiral arms or significant dust lanes. The galaxy exhibits an elliptical shape, displaying more length than width. There are no obvious signs of a major ongoing merger or strong tidal disturbances, though the shape is not perfectly regular.
