The galaxy presents as a spiral type, with a bright, somewhat amorphous central bulge. Spiral arms are observed, exhibiting a tightly wound morphology. The arms display a mottled texture, suggesting regions of active star formation, though the resolution limits a precise assessment of individual star-forming regions. There appears to be two spiral arms emerging out of the central bulge. The overall color index suggests a relatively evolved stellar population, although some bluer regions indicative of younger stars are also present. There is no obvious indication of strong tidal disturbances or ongoing major merger activity, however there are indications of minor disturbances. Dust lanes may be present but is obscured by resolution.
