The galaxy presents as a somewhat elliptical, though mostly round, structure. A prominent central bulge exhibits a yellowish hue, suggesting an older stellar population. The outer regions appear bluer, possibly indicative of younger stars and ongoing star formation, though at a low rate. The overall morphology appears relatively undisturbed, with no major signs of tidal interactions or ongoing mergers. There may be slight disturbances but none prominent enough to be called a merger. The overall form exhibits a fairly smooth distribution of light, but there is a very slight disk-like presence.
