The galaxy appears as a diffuse, elliptical-like structure with a relatively smooth light distribution. A concentrated central region shows the brightest luminosity, suggesting a high stellar density in the core. There is a hint of structural asymmetry or a potential tidal disturbance extending towards the left side of the image, possibly indicative of an interaction or past merger event. Overall, the galaxy appears to be in an intermediate stage of morphological transformation, displaying a mix of features associated with both elliptical and potentially spiral morphologies affected by interaction. The colors indicate intermediate to old stellar populations dominating the light, with potentially ongoing but low levels of star formation as suggested by the presence of bluer regions.
