The galaxy presents as a relatively compact object with a smooth, somewhat amorphous appearance. There is a discernible central bulge, characterized by a yellowish-orange hue, suggesting an older stellar population. The disk component, extending outwards from the bulge, exhibits a bluer color, indicating the presence of younger, hotter stars and potential ongoing star formation, albeit at a moderate rate. The overall shape is somewhere between round and elongated. There is a possible indication of a minor disturbance in the galaxy's morphology, hinting at a past interaction or minor merger event, but the majority of the galaxy appears relatively undisturbed.
