The galaxy presents an overall elliptical morphology, appearing elongated rather than spherically symmetric. It exhibits a smooth, relatively featureless structure, with no prominent spiral arms or bar structures readily discernible. There is a central concentration of light, suggesting a prominent bulge or core region.

The color gradient transitions from a more yellow/orange hue in the center to a bluer tinge in the outer regions. The central region appears to be dominated by older stellar populations emitting in the redder wavelengths. The bluer color in the outer regions could indicate the presence of younger, hotter stars, or possibly some ongoing star formation, albeit subtle. There may be a disk structure present.

Overall, the galaxy appears relatively undisturbed. There is a lack of obvious signs of major mergers or tidal interactions, although some subtle asymmetries in the outer regions hint at possible minor disturbances.
