This galaxy presents as an elliptical morphology, elongated with an approximate axis ratio of 0.5. A smooth and diffused light profile dominates the galactic structure. There is a central, concentrated region of heightened luminosity. Moving outward from the center, the galaxy gradually fades in intensity, demonstrating no distinct spiral arm features. A subtle color gradient is observed, with the central bulge exhibiting a slightly yellowish or golden hue, suggesting an older stellar population. The outer regions appear somewhat bluer, potentially indicating pockets of younger stars or ongoing, though subdued, star formation activity. However, signs of star formation are relatively subdued. No clear signs of tidal disturbances or merging events are apparent in this image, indicating it is likely a relaxed system. The Sersic index is approximately 1.0, supporting the notion of a disk-like galaxy.
