The galaxy presents a primarily smooth, somewhat elliptical morphology. The light distribution appears centrally concentrated with a bright, compact core region, suggestive of an active galactic nucleus or a dense stellar population. Moving outward from the core, the light gradually decreases, displaying a more diffuse halo. Subtle structural features are visible in the outer regions of the galaxy, indicating potential tidal disturbances or minor interactions. The galaxy exhibits a blue hue, which implies active star formation, possibly with a high population of young, hot stars. 
