The galaxy presents as a centrally concentrated system with a smooth appearance and a blue-shifted hue. The core exhibits a high degree of spheroidal symmetry. Evident is a lack of distinct spiral arms or a well-defined galactic disk. There may be minor tidal disturbances or a very faint structure to one side, suggesting a possible minor interaction or recent accretion event, however this is difficult to confirm. The light profile indicates a mature stellar population, with ongoing star formation. The system’s color suggests a relatively high rate of star formation, placing the galaxy within the star-forming main sequence. Overall, the galaxy morphology resembles that of an elliptical galaxy, possibly undergoing a minor interaction or experiencing increased star formation for an elliptical.
