The galaxy presents a primarily smooth morphology, with a concentrated central bulge. Evidence suggests a possible disk-like structure, although it is not sharply defined. The galaxy appears to be a flattened ellipsoid, exhibiting a shape somewhere between round and elongated, but not significantly cigar-shaped. No signs of major mergers or significant tidal disturbances are immediately apparent. The color profile indicates a population of older stars, particularly within the bulge region. The galaxy does not appear to be undergoing vigorous star formation. Overall, the galaxy resembles a relatively undisturbed disk galaxy with a prominent bulge.
