The galaxy presents as a relatively luminous system. It appears as an elliptical galaxy, with a pronounced bulge and a fainter, more diffuse halo. The bulge exhibits a yellow-red hue suggesting an older stellar population, while a bluer component extends outward, potentially indicative of ongoing star formation or a younger stellar population.

The morphology suggests the galaxy might be undergoing an interaction or merger. An extended tidal feature projects outwards from the main galactic body. This tidal tail appears blue, further suggesting recent star formation possibly triggered by the interaction. The main body exhibits a flattened shape.

Based on the colors, the galaxy likely has a moderate amount of dust obscuring some of the central regions. The outer regions are less affected and appear bluer.
