The galaxy presents a generally smooth morphology, with a dominant, centrally concentrated bulge region. The bulge exhibits a yellowish-white hue, potentially indicative of an older stellar population. Surrounding the bulge is a faint disk component, showing a bluer coloration which suggests the presence of younger stars and ongoing star formation. The overall shape of the galaxy appears to be approximately elliptical, verging on being spheroidal. There are subtle irregularities in the outer regions of the disk which could be very minor tidal disturbances or internal structural features. No prominent spiral arms or significant dust lanes are apparent within the visible light data. The galaxy is moderately luminous and has a substantial stellar mass.
