The galaxy presents as a lenticular or possibly an elliptical type, exhibiting a smooth, centrally concentrated light profile with minimal discernible structure in the visible bands. Its overall shape appears elongated, with the major axis significantly exceeding the minor axis. There is a distinct bulge, and evidence of a disk structure. The galaxy's color index suggests a population of older stars, consistent with a relatively low star formation rate. No prominent dust lanes or spiral arms are visible. There might be a faint halo or extended envelope.