The galaxy presents a primarily smooth, elliptical morphology with a high degree of central concentration. There is very little evidence of spiral arm structure or significant dust lanes. Its overall shape appears somewhat oblong, leaning towards an "in-between" classification rather than perfectly round. The color profile suggests a galaxy dominated by older stellar populations, as it exhibits a yellow-red hue across its body. There is no clear indication of ongoing major mergers or tidal disturbances impacting the galaxy's overall structure, though there is the possibility of minor disturbances to the side of the galaxy. The galaxy has a measured diameter of approximately 4.7 kpc. 
