The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. A bright, compact core is visible, surrounded by a more diffuse, extended halo. There's a subtle color gradient, with the central region appearing yellower, potentially indicating an older stellar population or significant dust obscuration. Fainter bluish light is observed in the outer regions, possibly indicative of more recent star formation within the galaxy's disk. There is little evidence of strong spiral arms or significant tidal disturbances, suggesting it is a fairly settled system that is not currently undergoing a major merger event. The overall structure suggests a relatively evolved galaxy with a moderate amount of star formation occurring within its disk.
