The galaxy exhibits a somewhat amorphous morphology, dominated by a smooth, spheroidal component. While a distinct disk structure is not clearly observed, there appears to be some evidence of subtle, disturbed features. There is a suggestion of an ongoing or recent merger event, possibly with interactions causing tidal disturbances within the galaxy's structure. The galaxy displays a relatively concentrated central brightness, with a gradual decrease in luminosity towards its outer regions. The overall color of the galaxy appears relatively red, possibly indicating an older stellar population with lower current star formation. The overall structure is somewhat round.
