The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge that transitions into a diffuse halo. The central bulge displays a yellowish-orange hue, suggestive of an older stellar population. The outer regions of the galaxy appear bluer, perhaps indicating the presence of a younger population of stars or some recent star formation activity, however this activity is faint. There are no readily apparent spiral arms or significant dust lanes. The galaxy possesses a near-spherical morphology, though some slight deviation from perfect roundness cannot be excluded. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. The galaxy appears to be a relatively isolated system exhibiting characteristics of an early-type galaxy.
