The galaxy presents as a single, relatively smooth, and centrally concentrated light distribution. It is largely elliptical in appearance, exhibiting a high degree of circularity with no apparent disk features. The color profile transitions from a warmer, yellower hue at the core to a cooler, greenish-blue periphery. There is no evidence of strong spiral arm structure or significant dust lane obscuration. No other object appears to be tidally disrupting the shape, suggesting that it is not undergoing a major merger. The overall morphology suggests a passively evolving galaxy, consistent with a relatively low star formation rate.
