The galaxy presents as a roughly circular, concentrated object. Its light profile appears smooth and lacks any distinct spiral arms or bar-like structures. The core exhibits a brighter, more intense luminosity, suggesting a possible active galactic nucleus or a high concentration of stars in the galactic center. There is minimal evidence of disk-like structures or significant features. The galaxy appears to be relatively isolated, without obvious signs of tidal interactions or major mergers. The overall appearance suggests a spheroidal or elliptical galaxy type, rather than a spiral galaxy. A slight asymmetry may be present in the outer regions, but further analysis is required to determine if this is a genuine feature of the galaxy or a result of observational artifacts.
