The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated, smooth light distribution with a significant fraction of the light concentrated towards the center. A noticeable radial gradient in surface brightness is present, transitioning from a bright, almost stellar-like core to a diffuse halo. There is a slight elongation observed; however, the shape is more lenticular than cigar-shaped. It does not appear to be undergoing any major merging activity, although there appears to be a minor disturbance on the edges of the disk. The galaxy displays colors that are consistent with an intermediate redshift with moderate star formation. The galaxy appears to be a relatively high mass.
