The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a gradual decrease in surface brightness from the core outwards. The core appears a yellow-white hue, indicative of an older stellar population dominating the central regions. The galaxy's overall shape is elongated, with a noticeable deviation from perfect circularity. There is faint evidence of a disk or extended structure, although it is poorly defined and subtle. The colors suggest low-level ongoing star formation, but is dominated by older, redder stars. No distinct spiral arms, bars, or dust lanes are visible. The light distribution suggests a relatively undisturbed system with no signs of recent major mergers or interactions. Overall, the galaxy appears to be a relatively evolved system.
