The galaxy presents as a relatively smooth, elliptical-like structure with a slightly elongated morphology. The central region exhibits a high surface brightness, suggesting a dense concentration of stars. The color gradient transitions from a bright yellowish-white core to a fainter, more reddish halo. There are no readily apparent spiral arms or significant dust lanes visible in this image. Based on the light profile, the galaxy appears to be dominated by an older stellar population, consistent with an early-type galaxy classification. There are no visible signs of major merger events or significant tidal disturbances.
