The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. There is a noticeable lack of well-defined spiral arms or a prominent disk structure. The central region appears brighter and more condensed, suggesting the presence of a galactic nucleus. The outer regions exhibit a gradual decrease in luminosity, fading into the background.

There is some evidence of a possible minor disturbance or interaction occurring, with subtle asymmetries in the galaxy's overall shape, potentially caused by a past or ongoing merger event. The galaxy exhibits a relatively blue hue in the g-band, indicating the presence of some star formation, but it is not vigorously star-forming.
