The galaxy presents as a somewhat elongated structure with a notable central bulge. The bulge exhibits a yellowish-white hue, suggesting a population of older stars. Fainter, bluer regions appear to extend outwards from the bulge along the longer axis of the galaxy, potentially indicating the presence of younger stellar populations and ongoing star formation within a disk-like structure. The galaxy doesn't exhibit any obvious spiral arm structure; the disk appears somewhat amorphous. The overall shape of the galaxy is somewhat cigar shaped. There is no obvious major disturbance indicating a recent major merger. The galaxy appears to be relatively isolated with no signs of interaction with any nearby galaxies.
