The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and concentrated light profile. It displays a noticeable bulge component which is generally yellowish, suggesting an older stellar population. The surrounding disk, if present, is faint and somewhat bluish, potentially indicating more recent star formation, even though it appears subdued. The overall shape is elongated, falling somewhere between round and cigar-shaped. There are no obvious signs of major mergers or tidal disturbances, and the overall structure appears relaxed, with no strong evidence of spiral arms or significant dust lanes. Overall, the galaxy presents a picture of a relatively evolved system.
