The galaxy presents as a moderately bright, fairly compact, and smooth elliptical. Its core is bright and yellowish suggesting an older stellar population. The galaxy lacks any clear spiral arm structures or significant dust lanes. There is a slight fall-off in intensity from the center, which has a golden hue, to the outskirts of the galaxy, where the color seems to be slightly redder. This color gradient may indicate radial variations in stellar age or metallicity. There are no obvious signs of recent major merger activity, but minor disturbances may be present in the galaxy's shape. Overall, the galaxy seems to be a relatively quiescent system.
