The galaxy presents as a fairly smooth, disk-like structure with a central bulge. It exhibits an elongated, cigar-shaped morphology, suggesting an elliptical or lenticular classification. The core region appears to be comprised of older stars, indicated by the yellowish-orange hue. A bluer, diffuse halo surrounds the central region, possibly indicating younger stellar populations or ongoing star formation within the disk. There is no visible evidence of spiral arm structure or major disturbances due to mergers. The overall structure suggests a relatively evolved system with limited recent interaction.
