The galaxy presents as an elongated, cigar-shaped system with a smooth, featureless morphology. A concentrated central bulge dominates the luminosity profile, appearing a yellowish-white hue, suggesting a population of older stars. Fainter, bluer emission extends along the major axis, tracing a flattened disk structure. The smooth appearance indicates a galaxy dominated by an evolved stellar population with a relatively low star formation rate. There is no obvious evidence of spiral arms, strong dust lanes, or ongoing major mergers. Minor disturbances cannot be ruled out given the resolution.
