The galaxy presents as a centrally concentrated object with a generally smooth appearance. It displays a slightly elliptical morphology, deviating marginally from a perfectly circular shape. The central region exhibits a brighter, more condensed luminosity profile that fades gradually into the outer regions of the galaxy. There is a subtle indication of a disk-like structure, but the overall texture appears largely featureless, which suggests it may be undergoing little active star formation. The light emitted is yellowish, indicating an older stellar population with less of the blue light we see in the more active galaxies. There seems to be little to no evidence of a major merger or significant tidal disturbance.
