The galaxy appears as a somewhat smooth, lenticular-like object. It exhibits a concentrated central bulge that seems to slightly dominate the overall structure. The galaxy is not perfectly circular, but is more of an in between shape. There is no obvious spiral arm structure or distinct features that are immediately apparent, though some subtle irregularities suggest minor gravitational disturbances, which could indicate ongoing or past minor merger events. Color gradients across the galaxy are subtle, with a slightly bluer hue in the outer regions compared to the more reddish central bulge.
