The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, featureless morphology. Its shape is moderately elongated. The central region displays a higher luminosity concentration, indicating a likely prominent galactic nucleus. The galaxy's color gradient suggests a higher concentration of older stellar populations, likely with reduced star formation within. There are no readily apparent signs of spiral arms, dust lanes, or significant tidal disturbances, suggesting it is not currently undergoing any major merger events, though there is a small suggestion of a minor disturbance. 
