The galaxy presents a predominantly smooth and rounded morphology. The central region exhibits a concentrated, bright core, indicative of a significant stellar population or possible active galactic nucleus. The overall color profile appears to be relatively red, suggesting a population of older stars and/or significant dust obscuration. There's very little indication of spiral arms, bars, or other distinct features typically associated with actively star-forming disk galaxies. Subtle color variations are visible in the outer regions, hinting at either patchy dust distribution or variations in stellar population. Based on its roundness, color, and lack of visible spiral structure, it likely belongs to the elliptical galaxy class. There is no indication of interaction with another galaxy.
