The galaxy presents as a slightly elongated, elliptical form with a concentrated central bulge. The bulge exhibits a yellow-orange hue, suggestive of an older stellar population. The surrounding disk shows a bluer color, indicative of younger stars and possible ongoing star formation. A subtle asymmetry may be present in the outer regions of the disk. The smooth appearance suggests it may be an early-type spiral galaxy. There's little indication of any major mergers or significant tidal distortions.
