The object appears to be a spiral galaxy viewed nearly edge-on. There is a prominent central bulge that appears yellowish-white in color, possibly indicating an older stellar population. The disk of the galaxy is visible as a flattened structure extending outwards from the bulge. It exhibits a bluish tint, particularly toward the outer edges, possibly indicative of ongoing star formation within the spiral arms. The galaxy does not exhibit any major signs of disturbance such as tidal tails or irregular shapes, suggesting a relatively isolated and quiescent system. No obvious bar structure is apparent. The galaxy appears relatively smooth, without prominent knots or HII regions visible in the disk.
