The galaxy exhibits a flattened, disk-like morphology with a noticeable central bulge. It is elongated, appearing somewhere between round and cigar-shaped. The central region displays a bright, yellowish-white glow, suggesting a concentrated population of older stars. A bluer, fainter halo surrounds the core, implying the presence of younger stellar populations and possibly ongoing star formation, though at a relatively low rate. There are no indications of a recent major merger or significant tidal disruption evident in the image; however, the presence of some minor disturbances cannot be ruled out. The overall smoothness of the galaxy indicates that it is likely an early-type spiral or a lenticular galaxy, with a prominent bulge and a relatively quiescent disk.
