This galaxy appears to be a spiral galaxy, observed at an angle. The central bulge is bright and concentrated, exhibiting a smooth, yellowish-white color indicative of an older stellar population. From the bulge, a single, well-defined spiral arm extends outwards, displaying a bluer hue compared to the bulge. This color suggests the presence of ongoing star formation within the arm. The overall structure is relatively smooth, with a hint of some minor disruption, possibly from a past interaction. The size of the galaxy is relatively compact.
