The galaxy presents as an elliptical or lenticular type. It has a centrally concentrated bulge region with a yellowish-orange hue, indicating an older stellar population. The outer regions show a gradual decrease in luminosity, blending into the background sky. The overall morphology appears relatively smooth, with no apparent spiral arm structures or significant dust lanes visible in this image. The shape is elongated, suggesting a deviation from perfect circularity. There are no signs of major mergers or significant tidal disturbances. Based on color indices, star formation activity appears to be low.
