The galaxy presents an elliptical morphology, with an overall smooth appearance dominating its structure. A subtle disk-like feature or perturbation appears to be present, perhaps representing a minor interaction or internal instability. The central region of the galaxy exhibits a higher concentration of light, suggesting the presence of a bulge or nucleus. Color gradients are apparent, with the central region displaying a more red-yellow hue, indicative of an older stellar population or dust obscuration. The outer regions show a slightly bluer tint, suggesting the presence of younger stars, possibly from minor star formation activity. There is a faint asymmetry to the galaxy's shape, potentially indicating an ongoing or past merger event. The galaxy's size appears moderate.
