The galaxy presents as a luminous, centrally concentrated object with a generally smooth appearance. The core region exhibits a bright, yellowish-white hue, indicating a substantial population of older stars. The overall shape of the galaxy is elliptical, though it is not perfectly circular, appearing slightly elongated. There are hints of faint, diffuse extensions or a very subtle disk-like structure surrounding the central bulge. No prominent spiral arms or distinct dust lanes are apparent. The color gradient suggests a possible decline in star formation activity towards the outer regions. There appear to be no signs of any major ongoing merger events or significant tidal disturbances, although there is potentially a faint and minor disturbance present within the outer halo. 
