The galaxy presents as an elliptical morphology, elongated in shape with a cigar like appearance. The central bulge exhibits a yellowish hue, suggesting a population of older stars. Moving outward from the center, the color shifts towards a cooler, bluer tone, though there is less structure there. There are no distinct spiral arms or significant dust lanes visible. The light distribution appears relatively smooth, with little evidence of recent or ongoing major mergers, although a minor disturbance or potential interaction cannot be ruled out. Overall, the galaxy is relatively large, and has modest star formation.
