The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is generally well-defined, with a relatively smooth, diffuse halo. There are no visible spiral arms, bars, or prominent dust lanes within the galaxy, giving it a fairly regular structure. The galaxy displays a relatively uniform color profile across its visible extent, with no prominent color gradients or regions of intense star formation that would be indicative of a younger stellar population. There appears to be a slight extension, possibly a tidal feature or disturbance in the outer halo, however, this could also be due to artifacts. The galaxy is relatively undisturbed, and it appears to be an isolated galaxy that has not recently undergone a major merger. The galaxy does exhibit some elongation, with the major axis being slightly larger than the minor axis, suggesting it is not perfectly circular. 
