The galaxy presents as a moderately luminous, relatively compact system. It exhibits an overall elliptical morphology, appearing largely smooth with minimal discernible substructure or spiral arm features. The color gradient suggests a central concentration of older stellar populations, indicated by a yellowish-orange hue that gradually transitions to bluer tones in the outer regions. This suggests ongoing, though perhaps subdued, star formation at the galaxy's periphery. There is no obvious evidence of tidal interactions, strong asymmetries, or major disturbances, indicating the galaxy is likely in a relatively quiescent state. The galaxy's round shape suggests that it does not have significant angular momentum. 
