The galaxy presents as a system with a centrally concentrated, smooth morphology. A dominant, bright, yellowish core is apparent, exhibiting a gradual transition in luminosity outwards. The central region fades into a fainter, more diffuse halo extending outwards. The overall shape approximates a slightly elongated spheroid, with a moderate ellipticity. There is little evidence of distinct spiral arms or prominent dust lanes. Subtle color variations are noted, with the core exhibiting warmer tones compared to the slightly bluer periphery. The system shows minimal signs of recent major merger activity or significant tidal disturbances. The observed structure suggests a relatively evolved system.
