The galaxy presents as a relatively smooth, rounded elliptical. There is a subtle, apparent reddish hue indicative of an older stellar population. No clear spiral arm structure is discernible within the image resolution. There is no central bulge. There is a faint disk component visible. The galaxy appears undisturbed, with no evidence of ongoing major merger events or tidal tails. A slight asymmetry can be seen, which may indicate a minor merger.
