The galaxy presents a generally smooth morphology, exhibiting a slightly elongated, elliptical shape. A subtle color gradient is observed, with a hint of bluer tones towards the central regions and a gradual shift to redder hues in the outer regions. This could indicate a difference in stellar populations, with younger, hotter stars dominating the core and older, cooler stars populating the outskirts. There are no obvious signs of spiral arms or a prominent disk structure; any disk component would be relatively featureless. There are very faint hints of minor disturbances in the galaxy shape, perhaps due to a past interaction with a small companion, but it's overall structure suggests the interaction was minor.
