The galaxy appears as a relatively smooth, elongated structure. Its color profile indicates a dominant population of older stars, emitting primarily in the redder portions of the visible spectrum, with a hint of blue, suggesting some presence of younger stars. The galaxy's light is concentrated towards the center, with a gradual decrease in intensity towards the outer edges. It presents a cigar-like shape. There are no visible signs of spiral arms or distinct features, but the relatively smooth texture and the elongation suggest a disk galaxy viewed at an angle. No major disturbances due to mergers can be seen, there is no obvious tidal distortion or interacting companions.