The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. The isophotes appear generally rounded, tending toward a somewhat elliptical shape. There's little to no visible evidence of spiral arm structures or significant dust lanes. The outer regions of the galaxy fade gradually into the background sky, indicative of a diffuse halo component. No clear signs of active star formation are discernible from the image's color profile. Overall, the galaxy's appearance is consistent with that of a mature, early-type galaxy. There is a very slight asymmetry to the galaxy, which may be an artifact of image quality. The galaxy shows a slight elongation, with the major axis being about twice the size of the minor axis. There are no visible tidal tails or other features that would suggest a recent merger event, though the very slight asymmetry is difficult to characterize due to the galaxy's distance.
