The galaxy presents an elliptical morphology, although its structure is not perfectly spheroidal. The light distribution is generally smooth, suggesting an older stellar population. There is a notable central bulge where the intensity of light is high, and gradually decreases outwards. The galaxy exhibits a subtle blue hue, possibly indicative of ongoing, though limited, star formation. There appears to be a slight irregularity in the galaxy's morphology which may be the result of a minor interaction. The overall structure suggests the galaxy is not undergoing significant major merger activity. 
