The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the core, the color shifts towards a bluer tone, possibly indicating the presence of some younger stellar populations or ongoing star formation at a low rate within the disk. The overall shape appears mostly undisturbed with only minor visual asymmetry. There is no clear evidence of major tidal features or a recent merger event. The galaxy appears relatively isolated, without obvious signs of interaction with neighboring galaxies in the immediate vicinity. The outer regions gradually fade into the background sky, indicating a well-defined but diffuse galactic halo.
