The galaxy presents a predominantly smooth, elliptical morphology. There is little evidence of distinct spiral arm structure or significant dust lanes. The central region exhibits a high surface brightness, suggesting a dense concentration of stars. The galaxy appears mostly round in shape but may have a slight elongated feature. The color profile is relatively uniform, with a yellowish hue, indicative of an older stellar population and a low star formation rate. There is no visual indication of ongoing merger activity or major disturbances within the galactic structure.
