The galaxy presents as a moderately bright, elliptical or lenticular morphology. It exhibits a centrally concentrated bulge, which graduates outward into a fainter, more diffuse disk. The color profile suggests an older stellar population within the central bulge, indicated by the yellowish hue. The outer regions of the disk show subtle bluish tones, potentially hinting at more recent star formation activity, though it appears weak overall. No distinct spiral arms or bar structures are apparent, nor are any obvious signs of a major merger event such as tidal tails or significant morphological disturbance. The galaxy appears relatively undisturbed and evolved.
