The galaxy presents as a relatively smooth object, lacking any prominent spiral arms or bar structures. Its overall shape is elliptical, appearing mostly round and symmetrical. The central region exhibits a higher surface brightness, suggesting a concentrated nucleus or bulge. The color profile indicates a population of older stars with a reddish hue, while a faint blue halo suggests the presence of some younger, hotter stars towards the outer regions. There is no indication of any major ongoing merger activity, but there is a slight irregularity on the edge of the galaxy.
