The galaxy presents a somewhat diffuse and elliptical morphology. It appears to lack strong spiral arm structure, exhibiting a smoother, more homogenous distribution of light. The central region displays a higher concentration of luminosity, suggesting a prominent galactic bulge. The galaxy's color is generally muted, showing a slight color gradient from a yellower center to bluer outer regions, indicating a possible radial variation in stellar populations or dust content. There are hints of minor disturbances in the outer structure, but this could be due to image resolution. Overall, the galaxy appears to be in a state of relatively low star formation activity, consistent with a post-starburst or transitioning galaxy.
