The galaxy presents an elliptical morphology, appearing generally smooth with a centrally concentrated bulge. The light distribution suggests a moderate ellipticity, tending toward a cigar shape rather than being perfectly circular. The core is characterized by a bright, yellow-orange hue, implying a population of older, evolved stars. Fainter, greenish diffuse emission surrounds the central region, possibly indicative of some level of on-going star formation or ionized gas. There are no obvious signs of spiral arm structures or significant dust lanes. The overall structure appears relatively undisturbed, with no major tidal features or signs of a recent major merger.
