The galaxy presents as a moderately bright, relatively compact object. Its morphology appears predominantly smooth, exhibiting a centrally concentrated light profile. There is faint evidence of some bluer emission surrounding the central region suggesting the presence of a weak disk-like structure. The galaxy is more "in between" than perfectly round or cigar-shaped. No obvious signs of strong tidal interactions or ongoing major mergers are observed, though subtle irregularities may suggest minor disturbances. The galaxy displays a slight elongation, but the overall structure appears largely undisturbed.
