This galaxy appears to be a spiral galaxy, viewed at a somewhat oblique angle. The central bulge exhibits a yellowish hue, suggesting an older stellar population. Faint spiral arms are visible, showing subtle color variations, with regions of bluer light indicative of younger, hotter stars and ongoing star formation. The arms seem somewhat tightly wound. The overall shape leans towards a prolate spheroid, elongated along one axis. There's a possible minor disturbance or asymmetry in one of the spiral arms, suggesting a past interaction or minor merger. The galaxy appears relatively isolated, showing no signs of a major ongoing merger or tidal features.