The galaxy presents as a relatively smooth, elliptical morphology. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish hue suggesting a population of older stars. The outer regions display a fainter, more diffuse halo. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's overall color suggests a relatively low rate of ongoing star formation. The shape appears somewhat elongated, with a moderate ellipticity, not exhibiting a perfectly circular profile. There are no obvious signs of major mergers or significant tidal disturbances in its immediate vicinity, though some minor asymmetry cannot be ruled out.
