The galaxy presents an overall smooth and round morphology, appearing largely featureless. A central, bright core region is evident, surrounded by a more diffuse halo of light. Color gradients suggest a subtle radial variation in stellar populations, with the core tending towards a more yellow/white hue, potentially indicating older stellar populations, while the outer regions exhibit a slightly bluer tinge, hinting at the presence of younger stars or ongoing star formation. The galaxy displays no apparent spiral arm structures or a prominent disk. There are some disturbances in the outer regions that could possibly be indicative of a minor merger or tidal interactions. Overall, the galaxy appears to be an elliptical galaxy undergoing minor interactions.
