The galaxy presents as a relatively compact, somewhat indistinct object. Its overall form appears roughly elliptical with an approximate radius of 1.75 arcseconds. The central region exhibits high luminosity, appearing nearly saturated in the image. This core luminosity decreases gradually towards the periphery, although the outer edges are not sharply defined. The color profile suggests a blue-shifted central region, possibly indicative of a younger stellar population or active galactic nucleus. The outer halo displays a reddish hue, potentially due to the presence of older, redder stars, or dust obscuration. There appears to be some asymmetry in the outer regions, hinting at possible minor tidal disturbances or interactions with other galaxies, or the result of a minor merger. No clear spiral arm structures are evident, and the galaxy seems to have a smooth texture overall. However, a slight distortion is observed, as if the galaxy is in the beginning of a collision with another object, and the core is not perfectly uniform.
