The galaxy presents an overall elliptical morphology, though there is some evidence of a disk-like structure. It exhibits a smooth appearance, with a relatively bright, concentrated central bulge. The outer regions appear less defined, fading gradually into the background. The light distribution is fairly even across the galaxy, with a color gradient apparent from the core outwards. The core shows yellow hues, suggesting the presence of older stellar populations, while the outer regions exhibit bluer tinges, implying the presence of younger stars and perhaps some ongoing star formation. There may be minor disturbances in the disk, but no strong evidence of a major merging event is readily apparent. Overall, the galaxy appears to be a transition type, between a purely elliptical and a spiral morphology.
