The galaxy presents as an elongated, ellipsoidal structure. It exhibits a smooth, centrally concentrated light profile, with a noticeable color gradient shifting from redder hues towards the core to slightly bluer tones in the outer regions. The ellipticity is significant, suggesting it is a highly inclined disk or an elliptical galaxy. There is no discernible spiral arm structure or bar feature evident in this image, and there are no signs of any major disturbances or ongoing merging activity. The primary color distribution appears to be fairly uniform across the galaxy's body, with only subtle variations in the observed color gradients.
