This galaxy presents as a largely featureless, elliptical-like structure. The light is concentrated towards the center, which has a distinctly orange-red hue. The radial color gradient suggests a redder stellar population becomes more dominant towards the core. The outer regions exhibit a subtle decrease in surface brightness and appear smoother and more diffuse than the central region. Faint, somewhat irregular structures, potentially representing tidal features or faint spiral arms, are suspected but difficult to confirm given the overall smoothness and lower resolution. There is no evidence of a strong, recent merger. The overall morphology suggests a relatively evolved galaxy with a low star formation rate. The estimated size is roughly 3.7 kpc based on estimated radius. The shape deviates somewhat from perfectly round, displaying slight elongation.
