The galaxy presents as an elongated, disk-like structure, likely viewed edge-on. The central region exhibits a concentrated, bright yellowish-white bulge, suggesting a significant population of older stars. Extending outward from the bulge, faint bluish-white light indicates the presence of a disk component. The distribution of light within the disk appears somewhat uneven, possibly suggesting spiral arm structures, though these are not clearly defined. The outer edges of the disk fade gradually into the background. There is some indication of potential tidal disturbances or asymmetries in the disk, but the galaxy appears relatively undisturbed overall.
