The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution is centrally peaked, with the brightest region appearing a warm yellow-orange hue, indicative of an older stellar population. The overall shape is close to round, exhibiting minimal ellipticity. There is no obvious disk component or spiral arm structure. The outer regions appear more diffuse and exhibit a bluer color than the core, possibly indicating a younger stellar population within the galaxy's halo. There is no apparent major interaction or merger activity significantly disrupting its morphology, however there may be slight morphological disturbance within the central region.
