The galaxy presents as a centrally concentrated, luminous object with a generally smooth appearance. It exhibits a somewhat elliptical morphology, although not extremely elongated, appearing more 'in-between' a circular and cigar shape. The central region displays a yellowish hue, indicating a potentially older stellar population. Fainter, bluer light extends outwards from the central region, suggesting the presence of some younger stars or ongoing star formation at the galactic outskirts, though this activity appears to be relatively subdued overall. There's a slight indication of minor disturbances in the outer regions, possibly suggestive of a past interaction or merger event. The overall structure gives the impression of a mature system, possibly an early-type spiral or lenticular galaxy, with a dominant bulge component and a fainter, less prominent disk.
