The galaxy presents as a somewhat elliptical, though close to round, structure with a smooth, diffuse appearance. The central region exhibits a yellowish-white color, suggesting an older stellar population. Moving outward from the center, the color gradually transitions towards a bluer hue, particularly on one side. This bluer region may indicate areas of more recent star formation. There appears to be a slight tidal feature or merging partner with a blueish red color that might indicate new star formation or gas compression due to gravitational interactions. The overall morphology suggests a galaxy undergoing some form of gravitational interaction or disturbance. The relatively smooth profile hints at a later-type galaxy, but one that has possibly experienced some form of dynamical evolution leading to the observed features.
