The galaxy presents as a moderately bright, centrally concentrated object. Its overall morphology is elliptical, exhibiting a smooth luminosity profile that decreases gradually with increasing radius from the core. The core region is defined by a yellow/white hue, indicating the presence of an older stellar population. There is a slight extension to the shape that is difficult to define given resolution. Fainter blue color is present in the outer regions, hinting at regions of ongoing, albeit potentially minimal, star formation. There is no apparent spiral structure or disk component. There is no sign of any major mergers, but there are possible minor disturbances.
