The galaxy presents as a somewhat elliptical object with a smooth appearance, exhibiting a central bulge that dominates the overall structure. The core region demonstrates a high concentration of light, gradually decreasing in intensity towards the outer regions. The observed color profile suggests a population of older stars, possibly with a limited amount of on-going star formation in the disk. No distinct spiral arms or significant dust lanes are readily apparent, pointing toward a more evolved system. The galaxy has a reddish hue, implying a low to moderate redshift.
