The galaxy appears to be a relatively smooth, elliptical type. It presents a centrally concentrated brightness profile with a gradual decrease in luminosity towards the outer regions, indicating an older stellar population. The galaxy exhibits a slightly elongated shape, transitioning from round to cigar shaped. There is no apparent spiral structure or prominent dust lanes visible. The galaxy appears undisturbed, without any signs of ongoing major merger activity or significant tidal distortions. The color is relatively homogenous throughout the galaxy, with a slight shift towards redder hues, suggesting a low rate of recent star formation. The galaxy exhibits no signs of an active galactic nucleus based on this image.
