The galaxy appears as an elliptical or lenticular type with a smooth, featureless morphology. There is a centrally concentrated bulge that dominates its light profile. The object presents with an overall yellowish-white color, suggesting a stellar population dominated by older, redder stars. No spiral arms or dust lanes are discernible. The galaxy exhibits a roughly circular shape, with only a slight deviation from perfect roundness. There is no evidence of ongoing major mergers or significant tidal disturbances, although a minor interaction cannot be ruled out. The galaxy appears relatively isolated within its immediate environment. The estimated effective radius of the galaxy is approximately 4 kpc.
