The galaxy presents as a single, centrally concentrated object with a fairly smooth overall appearance. Its shape is generally elliptical, appearing mostly round with a very slight deviation towards a cigar shape. A bright central bulge dominates the structure, exhibiting a concentrated luminosity. The outer regions of the galaxy demonstrate a gradual decrease in surface brightness, without any clear signs of distinct spiral arms or intricate features. There is no strong indication of major merger activity, but a very minor disturbance cannot be ruled out entirely. The galaxy has a reddish-yellow hue, possibly indicating an older stellar population with relatively low star formation.
