The galaxy presents an overall elliptical morphology, with a smooth light distribution. It is elongated, but not extremely so, exhibiting an intermediate roundness. The central region displays a higher surface brightness, suggesting a concentrated nucleus. The color profile appears to be relatively uniform across the galaxy, with a slight shift towards redder hues in the central bulge and bluer hues in the outer regions. No distinct spiral arms or prominent dust lanes are visible. There is no evidence of any major ongoing merger events or significant tidal disturbances.
