The galaxy presents an elliptical morphology. It exhibits a centrally concentrated bulge with a smooth, diffuse halo. The light distribution transitions gradually from the bright central region to the fainter outer regions, indicating a lack of distinct spiral arms or other prominent features. The core region presents a yellowish color, suggestive of an older stellar population. Proceeding outwards, the galaxy exhibits a slight shift towards redder hues. The overall shape is roughly circular in projection, with only a slight deviation suggesting some elongation. There are slight irregularities in the light distribution, potentially indicating tidal disturbances. No obvious signs of a recent major merger are apparent, though a minor interaction could be plausible.
