The galaxy presents as a largely featureless, elliptical-like structure. The central region exhibits a concentrated, bright, yellowish-white luminosity. This suggests a significant population of older stars. The outer regions display a gradual decrease in intensity, fading into a less defined halo. The overall smooth appearance indicates a morphological classification leaning towards an early-type galaxy, possibly an elliptical or lenticular. There is a slight irregularity in the outer isophotes which may suggest minor disturbances, possibly hinting at a past or ongoing minor merger event. Overall, the galaxy appears to be relatively isolated and undisturbed, based on the absence of any prominent tidal features.
