The galaxy presents as a relatively smooth, elliptical-like structure. A bright, concentrated central bulge is visible, surrounded by a fainter, more diffuse halo. There is a slight elongation to the galaxy's overall shape. Little evidence of spiral arm structure or significant dust lanes is apparent in this imaging. Subtle color gradients exist, with the central bulge exhibiting a yellowish hue, potentially indicating an older stellar population, while the outer regions appear slightly bluer, perhaps suggesting more recent star formation. The galaxy seems to be largely undisturbed, showing no signs of major mergers or tidal interactions.
