The galaxy exhibits a lenticular, disk-like morphology, observed nearly edge-on. A prominent bulge is visible, concentrated towards the center, and it is generally round in shape. A flattened disk component extends outwards. The disk appears smooth, with very little resolved structure. The galaxy presents a color gradient, transitioning from a yellowish-white hue in the central bulge to a slightly bluer tint towards the outer regions of the disk. There are no visible signs of tidal tails, distorted morphology, or other major disturbances suggestive of recent major merger activity, although minor asymmetry may be present. The galaxy is relatively isolated in this field of view.
