The galaxy presents as a moderately luminous, disk-shaped system with a dominant, spheroidal bulge. The bulge exhibits a yellow-white hue, suggesting an older stellar population. The disk surrounding the bulge displays a bluer color profile, hinting at ongoing star formation. The galaxy's overall morphology appears relatively smooth and undisturbed. The disk is slightly inclined relative to our line of sight, but it is difficult to identify any distinct spiral arms. There may be evidence of minor interactions or disturbances within the galaxy's outer regions, but the bulk of the object shows no indication of major ongoing mergers. The disk's outer region shows signs of blue light, possibly representing star formation. The galaxy's red shift puts it at a considerable distance. Overall, the galaxy seems to be intermediate between spiral and elliptical morphology.
