The galaxy presents an overall disk-like morphology, appearing relatively compact with an estimated angular size of approximately 7 arcseconds. The central region exhibits a strong, bright core indicative of a luminous galactic nucleus. Surrounding the nucleus, the galaxy appears to have a flattened disk structure oriented approximately horizontally in the image.

The color gradients across the galaxy suggest varying stellar populations and dust content. The central bulge region shows bluer hues, potentially indicating younger, hotter stars, while the outer disk appears to contain a mix of colors. There may be evidence of minor tidal disturbances in the outskirts of the galaxy, though the overall form remains largely undisturbed. No clear spiral arm structure is readily discernible.
