The galaxy appears to be a relatively smooth, elliptical galaxy. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density and potentially an active galactic nucleus, although further spectroscopic data would be required to confirm this. The isophotes appear roughly round with a slight elliptical deviation. There's no discernible spiral structure or prominent dust lanes. A subtle color gradient is observed, with a reddish hue dominating the central region, possibly indicative of an older stellar population, shifting toward a slightly bluer hue in the outer regions, hinting at the presence of some younger, hotter stars. No signs of any on-going major merger events or prominent tidal features are visible in the image. The light is fairly uniform, indicative of a fairly relaxed galaxy.
