The galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy. It exhibits a noticeable bulge, and a disk component is either absent or faintly visible. There are some faint, irregular features, possibly indicating minor disturbances or interactions. The overall shape is between round and elliptical, with no strong cigar shape. There is no clear sign of a major merger, but potentially a minor disturbance. The colors are relatively uniform, suggesting an older stellar population and limited ongoing star formation, with slightly more light in the redder bands. It is likely a galaxy of significant mass.
