The galaxy appears to be a somewhat elliptical, disk-like system. It presents a centrally concentrated bulge, indicated by a yellowish-white hue, suggesting an older stellar population dominates the core. Emanating from the central region is a fainter, bluish disk. The slight blue tint of the disk component indicates the presence of some younger stars or ongoing star formation. The disk is not uniformly colored and appears slightly disturbed in its shape. Overall, the galaxy presents a somewhat smooth appearance but possible merging activity is also present. The galaxy is moderately luminous.
