The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. Its overall morphology suggests a lack of spiral arms or a distinct disk structure. The central region is notably brighter and appears to be more yellow/gold in color, which might indicate a higher concentration of older stellar populations. The outer regions of the galaxy appear fainter and slightly bluer in color. There is no obvious ongoing major merging event, nor a large tidal tail. The galaxy appears fairly isolated, with no clear signs of recent interactions.
