The galaxy presents as an elliptical morphology, exhibiting a smooth and concentrated light profile. The central region displays a yellowish-white hue, suggestive of an older stellar population. There is a lack of prominent spiral arm structures or dust lanes. The galaxy's overall shape appears somewhat elongated. There is no evidence of tidal tails or significant distortions, indicating that the galaxy is likely undisturbed and not undergoing a major merger. Its color and smooth structure suggest a relatively quiescent system with low ongoing star formation activity. The galaxy exhibits a subtle color gradient, becoming slightly bluer towards the outer edges, potentially indicating younger stars or regions of recent star formation on the outskirts.
