The galaxy appears to be a relatively smooth, elongated, disk-like structure with a prominent central bulge. The color gradient suggests the bulge is comprised of older stellar populations, presenting a yellowish-white hue, while the outer disk displays a bluer tint, potentially indicating ongoing star formation. There is no evidence of prominent spiral arms or significant dust lanes. The overall form is quite regular, with no signs of major mergers or tidal disturbances, although a minor disturbance cannot be ruled out. The estimated physical size indicates this is a fairly large galaxy.
