The galaxy appears to be a lenticular or early-type spiral galaxy, viewed edge-on. It exhibits a smooth, elongated morphology with a noticeable central bulge that appears yellowish in color, possibly indicative of an older stellar population. Faint blue hues extend outward from either end of the major axis, suggesting the presence of some younger, hotter stars or potentially regions of ongoing star formation within a disk component. There appears to be only a small amount of disturbance present within the galaxy's structure. The system does not appear to be undergoing a major merger. Overall, the galaxy seems to be a relatively quiescent system.
