The galaxy presents a yellowish-white hue, concentrated centrally with a seemingly disrupted morphology. The core region appears brighter and more condensed, possibly indicating a higher density of stars or an active galactic nucleus. A fainter, diffuse halo surrounds the core, extending non-uniformly. The galaxy lacks a well-defined spiral arm structure, instead exhibiting a somewhat amorphous shape. There is evidence of potential tidal features or minor disturbances, possibly suggesting past or ongoing interactions with another galaxy, as indicated by the irregular shape and faint extensions. These features could point toward a merger event or gravitational interaction. There is no obvious dust lane visible. Overall, the galaxy's color suggests an older stellar population, though recent star formation may still be present.
