The galaxy presents as a somewhat symmetrical, moderately luminous object. It exhibits a prominent central bulge that appears roughly spherical. A diffuse halo surrounds the central region, with the light fading gradually towards the edges. The color profile suggests a relatively old stellar population in the core, indicated by the yellowish hue. The outer regions display a slightly bluer tint, suggesting the presence of younger stars or regions of ongoing star formation, although this is not strongly pronounced. There may be minor disturbances in the outer disk, but there is no definitive evidence of an ongoing major merger or tidal interactions. The general morphology is consistent with an early-type spiral galaxy, with a relatively smooth and centrally concentrated appearance.
