The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular classification. The central region exhibits a concentrated, bright core with a yellowish hue, indicative of an older stellar population. There is a hint of asymmetry in the outer regions, with some faint, diffuse extensions or tidal features visible. These features are bluer in color and appear to surround the central core. There may be a few compact regions of active star formation within the galaxy’s halo. Overall, the galaxy's structure suggests an evolved system with possible interactions or recent merger events.