The galaxy presents a predominantly smooth morphology, exhibiting a high degree of central concentration. There is a suggestion of a spheroidal shape. A very small, almost negligible amount of disk is present. The central region displays a distinct yellowish-orange hue, potentially indicating an older stellar population. Moving outward from the core, a subtle gradient is visible, transitioning to a fainter bluish halo. There is no clear evidence of spiral arm structures or significant dust lanes. Overall, the galaxy appears to be relatively undisturbed, with no strong indications of major mergers or tidal interactions.
