The galaxy appears as an elliptical or lenticular type, exhibiting a generally smooth morphology. The light profile suggests a centrally concentrated bulge that decreases gradually in intensity towards the edges. Its shape is more elongated than circular, appearing cigar-shaped with the major axis significantly longer than the minor axis. The galaxy displays a color gradient, trending from a yellowish-orange central region to slightly redder hues in the outer regions. There is no evidence of a strong spiral arm structure or prominent dust lanes within the visible light. There are no clear signs of a major ongoing merger or significant tidal disturbances.