This galaxy presents as a relatively smooth, elongated structure. The central region exhibits a concentrated, luminous core, appearing a warm yellow hue. This suggests an older stellar population dominates the core. Moving outward from the center, there's a discernible transition to a fainter, less defined disk-like structure. The disk's color shifts towards a bluer tone compared to the core, hinting at the presence of younger, hotter stars and potentially ongoing star formation within the disk. While the overall structure appears largely undisturbed, there is a subtle asymmetry in the outer regions. One side of the disk seems slightly more extended or diffuse than the other, which may suggest a minor interaction or disturbance. Overall, the galaxy appears as a relatively massive system, and a low star formation rate.
