The galaxy presents as a centrally concentrated, smooth object with a relatively round morphology. There is an apparent lack of defined spiral arms or a prominent disk structure. The central region exhibits a brighter, more intense luminosity, suggestive of a significant concentration of stars or possibly an active galactic nucleus. The outer regions of the galaxy appear more diffuse and fainter, gradually fading into the background. The color appears predominantly yellowish-white in the core, shifting towards a slightly bluer hue in the outskirts, potentially indicating varying stellar populations with age and composition. There's no immediately apparent evidence of ongoing major mergers or significant tidal disturbances, though subtle irregularities in the outer halo could suggest past minor interactions. The overall impression is of an evolved galaxy, likely an elliptical or lenticular type, exhibiting a smooth, generally undisturbed structure.
