The galaxy presents as an elliptical morphology. It exhibits a relatively smooth, symmetrical light distribution without prominent spiral arms or a distinct disk-like structure. The concentration of light is high towards the central region, with intensity gradually decreasing outwards. The overall color appears yellowish, suggestive of an older stellar population with relatively low ongoing star formation. There is no evidence of significant tidal disturbances, major mergers, or strong asymmetries. Close inspection reveals a possible minor perturbation within the galaxy's halo. The object presents an apparent size, corresponding to an estimated physical diameter of approximately 5 kpc.
