The galaxy exhibits a generally smooth morphology, with a relatively high degree of central concentration. The overall shape is close to round. There is no strong evidence of significant spiral arm structure or a prominent disk. Faint features are visible in the outer regions, suggesting possible faint disk structures or interactions. A slight ellipticity can be observed, but the object is largely circular. The color profile indicates that the central region is relatively brighter and has a yellow/white appearance, suggesting an older stellar population compared to the fainter, bluer hues in the outer regions. No obvious signs of a major merger or strong tidal disturbances are apparent, although subtle asymmetries might indicate a minor interaction in its past. 
