The galaxy presents a smooth, elliptical morphology. Its light profile appears concentrated toward the center, with a gradual decrease in intensity outwards. There is a distinct yellow-orange hue to the central region, possibly indicating an older stellar population. There is little evidence of prominent spiral arms or significant dust lanes. The galaxy's shape is somewhere between round and cigar-shaped, perhaps leaning slightly toward being in between those two. There are no obvious signs of major disturbances or ongoing mergers, although subtle irregularities might be present. Overall, the galaxy appears to be a relatively quiescent, evolved system.
