The object appears to be a spiral galaxy, viewed nearly edge-on. A prominent, somewhat bright central bulge is visible, displaying a yellow-orange hue, which may suggest a relatively older stellar population. The disk of the galaxy is thin and elongated, with a bluer color gradient towards the outer edges. The lack of readily apparent dust lanes suggests a relatively smooth distribution of interstellar material within the disk. The symmetry and defined bulge suggest that the object does not seem to be undergoing any major merging events, although there might be a slight disturbance or tidal feature extending from the disk. Overall, the galaxy exhibits characteristics consistent with a large, mature spiral galaxy. Star formation is expected to be minimal.
