The galaxy appears to be a lenticular or early-type spiral galaxy, viewed at a slight angle. It exhibits a prominent central bulge that appears yellowish-white, suggesting an older stellar population. A faint, diffuse disk extends from the central bulge. There may be hints of spiral arm structure embedded within the disk, but these features are not well-defined. The disk presents a bluer hue than the bulge, indicative of a younger stellar population and possible ongoing star formation. The overall shape of the galaxy is elongated, with a ratio of major to minor axis that suggests it is not viewed face-on. There is no evidence of major merger activity, although subtle disturbances in the disk structure cannot be ruled out.
