The galaxy presents as an elongated structure, suggesting an elliptical morphology or a disk galaxy viewed at an angle. The central region is significantly brighter and appears to be a yellowish-orange hue, potentially indicative of an older stellar population dominating the core. The outer regions are less defined, with a smoother, fainter gradient of light extending outwards. There is a slight bluer tint present in these regions. Overall, the galaxy appears relatively undisturbed, with no clear signs of major mergers or tidal distortions.
