The galaxy presents as a relatively smooth, elongated structure, likely an elliptical or lenticular galaxy viewed at an angle. The central region exhibits a yellowish hue, suggesting an older stellar population. Moving outwards from the center, a subtle color gradient transitions to a bluer periphery. This potentially indicates some ongoing, albeit subdued, star formation in the outer regions. The overall light distribution appears concentrated towards the center, fading gradually towards the edges. There is no obvious presence of spiral arms or a prominent disk. No signs of major mergers or significant tidal disturbances are visible.
