The galaxy appears as a relatively compact object. There is evidence of a bright central region, potentially a bulge or active galactic nucleus, with a surrounding disk or ring-like structure. The color gradients suggest variations in stellar populations or dust content across the galaxy. A slight asymmetry is observed. It's possible this galaxy is a spiral, seen at an angle, or it may be an elliptical object with some unusual dust and gas distribution. There may be evidence of a faint tidal tail or stream on one side, suggesting a potential gravitational interaction or minor disturbance. Further investigation is required to determine its morphological classification and interaction history.
