The galaxy presents a concentrated, smooth morphology. The light profile suggests a single, dominant spheroid structure. It appears elliptical with a moderate ellipticity, showing a shape somewhere between round and elongated. The color distribution exhibits a central concentration of redder hues, shifting toward a more uniform color profile at the outer regions of the galaxy, indicating a higher concentration of older stellar populations toward its center. There is no obvious spiral arm structure, strong dust lanes, or tidal features, suggesting this is likely not a recent merger event or a disk galaxy. A small amount of star formation might be present. The overall appearance indicates a relatively quiescent galaxy, possibly an early-type system nearing the red sequence.
