The galaxy presents as a fairly smooth, centrally concentrated object. It exhibits a bright, yellowish core that gradually fades into a more diffuse, bluish halo. There is little evidence of distinct spiral arms or a prominent disk structure. The overall morphology suggests a galaxy with a moderate redshift, potentially an elliptical or lenticular galaxy, but further spectral analysis is required to confirm its exact classification and evolutionary stage. There appears to be little to no major disturbance or ongoing merging activity. Faint, extended light suggests the presence of a stellar halo.
