The observed galaxy presents as a primarily smooth, disk-shaped structure viewed nearly edge-on. A central bulge is subtle, with light from a bright nucleus dominating the central region. The disk exhibits a color gradient, appearing bluer near the outer edges and transitioning to redder hues closer to the core. Evidence of spiral arm structures is minimal, though subtle asymmetries may be present along the disk. The galaxy displays hints of a potential minor disturbance or interaction based on slight irregularities and fuzziness, but it predominantly appears isolated and unperturbed. The color profile suggests active star formation in the outer regions.
