The galaxy presents as a somewhat elliptical, smooth object. The central region displays a yellowish hue, suggesting an older stellar population. Moving outwards, there is a subtle gradient toward bluer colors in the outer regions. This could be the presence of a younger stellar population within a disk-like structure. No distinct spiral arms or prominent dust lanes are visible. Overall, the galaxy exhibits a relatively undisturbed morphology, with no obvious signs of major mergers or tidal interactions. The galaxy appears to be relatively isolated, with no other galaxies in close proximity that could cause gravitational disturbances.
