The galaxy presents as an object with intermediate ellipticity, appearing neither perfectly circular nor elongated. Its overall structure is relatively smooth, with some indication of features possibly indicative of a disk. There are faint irregularities that might suggest minor gravitational disturbance, but no clear signs of an ongoing major merger event or strong tidal interactions. The light profile indicates a central concentration of light, characteristic of a galactic bulge or nucleus. Color gradients appear minimal across the galaxy's extent, suggesting a somewhat uniform stellar population or dust distribution. Overall, the galaxy appears as a relatively undisturbed, intermediate mass, early-type spiral or possibly an elliptical galaxy with subtle disk-like features. Star formation appears minimal.
