The galaxy presents a generally smooth and rounded morphology, with a centrally concentrated light profile. The color appears to be predominantly yellow and red, with subtle variations suggesting a relatively old stellar population. There is no strong evidence of spiral arm structure or significant dust lanes. The isophotes are generally regular, and the galaxy appears to be relatively isolated with no obvious signs of recent major merger activity. There may be some minor tidal disturbance visible. Overall, the galaxy appears to be consistent with an elliptical galaxy.
