The galaxy exhibits a centrally concentrated bulge with a smooth appearance, transitioning into a less defined, elongated disk. The disk is observed to be slightly inclined relative to our line of sight. The central region displays a yellowish hue, potentially indicating an older stellar population. Moving outwards from the core, the disk appears bluer, suggesting the presence of younger stars. The overall morphology leans towards a flattened spheroidal shape. There may be some low level disturbances to the galaxy.
