The galaxy presents a primarily smooth morphology, appearing elliptical in shape. The core region exhibits a high concentration of light, indicative of a significant stellar population. The color is predominantly yellow-white, suggesting an older stellar population with a lower rate of recent star formation. There are some hints of bluer tones within the galaxy, perhaps indicative of more recent star formation. There is no strong evidence of spiral arm structure or a prominent disk from this viewpoint. Minimal tidal distortion or interaction with nearby galaxies is apparent in the image, suggesting it is currently an isolated system. A subtle asymmetry in the outer regions might indicate a past merger event or ongoing accretion.