The galaxy presents as a somewhat elliptical, lenticular morphology. It exhibits a high degree of central concentration with a bright, yellowish core that fades smoothly outwards, suggesting a relatively old stellar population dominating the central bulge. The outer regions display a bluer hue, hinting at the presence of younger, hotter stars, possibly indicating ongoing or recent star formation at a low rate. The galaxy appears relatively smooth, with only subtle, diffuse features visible, without any strong evidence of spiral arms or significant dust lanes. There is no visual disturbance or signs of major interaction with other galaxies. The object seems to be of a significant size and mass. 
