The galaxy presents as a smooth, elliptical structure. Its overall shape is elongated, appearing cigar-shaped. The light profile suggests a concentration of older stars. There is no apparent evidence of spiral arms or significant dust lanes. The galaxy displays a reddish hue, possibly indicative of an older stellar population and relatively low star formation rate. Faint blue tinges are visible in the outer regions, hinting at some recent star formation. There is no clear indication of any major mergers or tidal disturbances affecting the galaxy.
