The galaxy presents as a smooth, elliptical-like object with a noticeable color gradient. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population dominated by redder giants and supergiants. Moving outwards from the core, the color transitions towards a bluer, fainter periphery. This suggests a possible presence of younger, bluer stars in the outer regions, though their contribution to the overall light is minimal. The light distribution is somewhat elongated, deviating from a perfectly circular morphology. There appears to be some level of disturbance, or potential interaction/merger that might be occurring. This could explain why its light seems to be asymmetric and patchy towards the outside of the galaxy.
