The galaxy presents a roughly elliptical morphology with a central bulge that is relatively bright and compact. The light from the galaxy appears smooth and somewhat diffuse, which suggests it is dominated by older stellar populations. There is a noticeable lack of well-defined spiral arms or prominent dust lanes.

The galaxy displays a bluer hue in its central regions, which is indicative of some ongoing, but not particularly vigorous, star formation. Fainter, redder outskirts indicate an aging stellar population at the edge of the galaxy. There may be a tidal tail or some minor morphological disturbance in the top left quadrant that could suggest a past or ongoing interaction with another galaxy, but the galaxy's smooth appearance suggests it is not undergoing a major merger.
