The galaxy presents as a centrally concentrated elliptical-like structure. The central region exhibits a smoother texture and a slightly reddish hue, possibly indicating an older stellar population. The outer regions display a bluer color, suggesting the presence of younger, hotter stars, potentially in a spiral arm structure, although these arms are not well defined and appear rather patchy. The galaxy's shape appears elongated with a smooth, less defined structure towards the center. There appears to be some minor disturbance or faint tidal features extending from the main body of the galaxy, indicating a potential recent or ongoing interaction with another galaxy or a minor merger event.
