This galaxy appears to be a spiral galaxy viewed at a high inclination. The central bulge exhibits a bright and smooth appearance. Faint spiral arms extend outwards from the bulge, primarily visible on the left side of the disk and less so on the right. The disk appears relatively thin, with no obvious dust lanes. The galaxy exhibits a bluish hue, suggesting the presence of younger stars. There is a hint of irregular structure, possibly indicating a past interaction or minor disturbance. Overall, the galaxy seems to be in a relatively undisturbed state, but the slight irregularity suggests potential ongoing or recent activity. The overall morphology leans towards a later-type spiral, where the bulge is less dominant.
