The galaxy presents as a single, relatively smooth concentration of light. The morphology appears largely elliptical, with no discernible spiral arm structure or prominent dust lanes visible in this image. The central region exhibits a bright, concentrated core, suggestive of a bulge or a possible active galactic nucleus, although this cannot be definitively confirmed from the available imagery. The galaxy's color index suggests a population of older stars. Star formation appears to be minimal or absent, judging by the lack of discernible blue regions indicative of hot, young stars. There is no evidence of major tidal disturbances or ongoing mergers in this image, though minor asymmetries or faint extensions might be present upon closer examination with higher resolution data. The galaxy's overall structure indicates it is a reasonably massive system.
