This galaxy presents as a somewhat centrally condensed object with an overall elliptical morphology. The core region exhibits a yellowish-white hue, suggesting a population of older, evolved stars. Surrounding the core, a less defined, diffuse halo extends outward. This halo appears bluer in color, hinting at the presence of younger stellar populations or ongoing star formation, although the rate of star formation appears to be relatively low. There is some evidence of minor disturbances in the outer regions of the galaxy, but no obvious signs of a major merger. It has a considerable mass. The shape is more in-between than cigar shaped or round. The galaxy appears mostly smooth.
