The galaxy presents as a moderately bright object with an apparent elliptical morphology. There is a subtle elongation noticeable in the image, though the overall shape appears fairly regular. Color gradients are present, with the central region exhibiting a yellowish hue, possibly indicating an older stellar population. The outer regions appear somewhat bluer, suggesting the presence of younger stars and ongoing star formation, albeit at a relatively low rate. There may be some faint tidal features or minor disturbances, possibly indicating a past interaction or minor merger event, however, the image quality limits clear identification. The galaxy exhibits a certain degree of smoothness, suggesting it is not a late-type spiral with prominent arms or a heavily disturbed system.
