This galaxy appears to be a relatively luminous, early-type galaxy, exhibiting a smooth, elliptical morphology. The light profile seems centrally concentrated, characterized by a bright, yellowish core that gradually fades into the surrounding halo. There is little evidence of spiral arms or significant dust lanes. The overall color is consistent with an older stellar population, hinting at a suppressed star formation rate within the galaxy. No signs of major mergers or tidal disturbances are apparent. The galaxy appears relatively isolated. The shape shows some ellipticity.
