The galaxy presents as a slightly elongated, lenticular object with a smooth, featureless morphology. The core exhibits a concentrated, bright, yellowish-white luminosity, suggesting a dense population of older stars. Progressing outwards from the center, the galactic disc displays a gradual decrease in luminosity. There is a subtle shift towards bluer hues in the outer regions of the disk, hinting at the presence of younger stellar populations or ongoing star formation, albeit at a low rate. The galaxy shows no evidence of spiral arm structures, significant dust lanes, or prominent tidal features. There are also no signs of any ongoing major merger events. A slight asymmetry in the outer regions may indicate a minor disturbance or past interaction with another galaxy, though overall, the galaxy appears relatively undisturbed.
