The galaxy appears to be a relatively small elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. The central region is the brightest, with the luminosity gradually decreasing towards the edges. It shows a nearly circular morphology, with only a slight elongation. There is a subtle color gradient, with the core appearing somewhat redder, possibly indicating an older stellar population, whereas the outer regions exhibit bluer hues, potentially suggesting the presence of younger stars or ongoing star formation at a low rate. The galaxy displays no obvious signs of spiral arms, dust lanes, or active galactic nuclei. The galaxy seems to be relatively isolated and undisturbed, showing no signs of major mergers or tidal interactions.
