The galaxy appears to be an elliptical galaxy, characterized by a smooth, featureless morphology. The galaxy exhibits a centrally concentrated light profile, with a gradual decrease in brightness towards the outer edges. The isophotes appear largely regular and elliptical. There is a lack of apparent spiral arm structure or prominent dust lanes. The color is relatively uniform and somewhat bluish, but with redder light at the edges, and a bright white core indicating the likelihood of intermediate age stars, with a very low rate of star formation. Based on the size and luminosity, it appears to be a smaller galaxy, with an estimated mass of somewhere around 10^9 solar masses. There does not appear to be evidence of any major merger events or significant tidal disturbances. There is a potential for a faint disc.
