The galaxy presents as a moderately elliptical, disk-dominated system seen at a significant inclination to our line of sight. It exhibits a bright, concentrated central bulge that dominates the luminosity profile. The bulge appears smooth and featureless. A flattened disk extends beyond the bulge, showing a slight warping. There is a subtle color gradient, with the central bulge displaying a yellow-white hue that transitions to a bluer tint towards the outer regions of the disk. This suggests ongoing or recent star formation in the disk. The overall structure is generally undisturbed, with no obvious signs of tidal features or major mergers. The galaxy appears to be relatively isolated, with no close companions immediately visible in the field.
