This galaxy appears as a relatively compact object. It exhibits a centrally concentrated luminosity profile, indicative of a bulge-dominated morphology. The galaxy displays a smooth overall appearance, lacking prominent spiral arms or other distinct features. There is a slight elongation, making it appear as being in between round and elliptical. I note red and green areas within the core of the galaxy, suggesting varying stellar populations or potentially differing levels of dust extinction across its structure. There are no obvious signs of tidal tails, strong interactions, or recent major merger events. However, there is a slight asymmetry in the outer regions that could indicate some degree of minor past interaction. Star formation appears to be relatively low within this system.
