The galaxy presents as a moderately bright object, appearing largely smooth with some subtle features. It exhibits a noticeable central bulge that dominates the overall morphology. The isophotes are elongated, indicating an elliptical or lenticular classification. There appears to be a faint and diffuse disk component extending outwards from the central bulge. A slight distortion is visible in the upper region of the disk, hinting at a possible tidal interaction or ongoing minor merger. The galaxy appears to have a redder color, indicating a population of older stars with subdued star formation.
