The galaxy presents as a relatively smooth, elliptical-like structure with a notable central bulge. Its color profile appears to shift from redder hues toward the core, possibly indicating an older stellar population concentrated centrally, to bluer shades in the outer regions suggesting the presence of some younger stars. The light distribution is fairly concentrated, with a gradual decrease in intensity moving outwards from the center. There's a subtle indication of minor disturbances in the outer arms. The galaxy doesn't appear to be undergoing a major merger, though slight asymmetries hint at past gravitational interactions. The shape is more in-between than distinctly round or elongated.
