The galaxy presents as a moderately luminous, early-type system. Its morphology is generally smooth with a slightly elliptical shape. The central region exhibits a significantly higher surface brightness, indicating a concentrated stellar population or possibly an active galactic nucleus, although the resolution is insufficient to confirm the latter. The color profile appears relatively uniform across the galaxy, suggesting an older stellar population with limited ongoing star formation. There is no visible dust lane or spiral arm structure. Some minor asymmetry may be present, however further investigation will be required to determine whether this indicates a past interaction or merger event. The galaxy appears to be relatively isolated.
