The galaxy presents as a slightly elongated, elliptical morphology. The central region exhibits a concentrated luminosity profile, suggesting a bulge-dominated structure. A subtle color gradient is observable, transitioning from a warmer, reddish hue near the apparent upper edge to a cooler, bluer tint at the opposite end. There appears to be some indication of disturbed morphology within the galaxy, which could potentially indicate past or ongoing minor interactions with another galaxy. No distinct spiral arm structures are readily visible in the image.
