The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a concentrated luminosity with a yellowish-orange hue. Extending outwards from this core, a distinct, yet somewhat diffuse, blue-ish region is observed. This region indicates the presence of ongoing or recent star formation. The overall structure appears relatively undisturbed with the exception of an arm-like protrusion. The galaxy exhibits a smooth, primarily elliptical morphology. The light distribution suggests a relatively evolved stellar population in the central bulge, while the bluer outskirts indicate a younger stellar population. The axial ratio suggests a highly inclined viewing angle.
