The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a noticeable radial decrease in luminosity outward. There are no clearly defined spiral arms or a prominent disk structure evident, though there may be a faint disk. There is a high likelihood of artifacts surrounding the galaxy, based on the light sources around it. 

Evidence suggests a minimal amount of merger activity, although there might be some minor tidal disturbance or signs of a recent or ongoing minor merger event that could be impacting the galaxy's overall shape.
