The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. It exhibits a somewhat elongated shape, appearing more "in between" round and cigar-shaped, though closer to round. There's minimal evidence of spiral arms or other distinct features.

The color profile suggests a dominant older stellar population. The core is noticeably brighter and concentrated, indicating a high stellar density. Based on color, the galaxy has low star formation rate. There does not appear to be any major disturbance or ongoing merger activity, rather it displays general smoothness.
