The galaxy presents an elliptical morphology, appearing as a smooth, somewhat elongated structure. It exhibits a concentration of light towards the center, indicating a bulge component. There is a subtle color gradient across the galaxy; the central region exhibits a yellowish hue, suggesting an older stellar population. The outer regions appear to be slightly bluer, potentially indicating the presence of younger stars or ongoing star formation, although not particularly intense. There is no visible spiral structure, distinct dust lanes, or any major disturbances indicative of a recent merger event. The galaxy does not appear perfectly round but is rather cigar-shaped. Overall, the galaxy seems to be a relatively undisturbed system.
