The galaxy presents an elliptical morphology, with a centrally concentrated, bright core that gradually fades into a more diffuse halo. Its overall color appears somewhat redder, indicating a population of older stars, likely with minimal ongoing star formation. The shape is neither perfectly spherical nor highly elongated, but is closer to in-between. There appears to be a very slight asymmetry to the galaxy, with a possible minor disturbance visible on one side. This could be indicative of a past or ongoing minor interaction or merger. However, there are no significant signs of tidal tails or highly distorted features, suggesting that any interaction has not been major. The galaxy appears smooth with very little structure, which would mean it would have a high smooth fraction. 
