The galaxy appears as a centrally concentrated object with an approximate diameter of 18 arcseconds. The central region exhibits a bright, intense luminosity, indicative of a high concentration of stars and potentially an active galactic nucleus. The overall color of the galaxy is bluish-white, which suggests the presence of a significant population of young, hot stars.

The galaxy presents subtle signs of irregularity in its morphology. Faint, diffuse extensions are seen extending from the main body, possibly indicative of tidal interactions or minor disturbances. These faint features appear more pronounced on one side of the galaxy, suggesting an asymmetry in its structure. There is no distinct spiral arm structure visible; instead, a more amorphous distribution of light is apparent. The outskirts of the galaxy are characterized by a gradual decrease in surface brightness, smoothly fading into the background.
