The galaxy presents as an elliptical or lenticular structure, appearing largely smooth with minimal discernible internal features. The galaxy exhibits a concentrated central bulge with a radial decrease in luminosity. There are no prominent spiral arms or bar structures observed. The overall color profile suggests a population of older stars, indicated by the yellowish-red hue dominating the core and extending into the outer regions. However, a small area of blue tinged light indicates possible recent star formation in the galaxy. There appears to be a possible minor tidal disturbance on the left of the galaxy. It does not seem to be undergoing a major merger event, although a close companion can't be ruled out from this image alone.
