The galaxy presents a predominantly elliptical morphology, exhibiting a smooth, concentrated central bulge that transitions into a more diffuse halo. The major axis is significantly longer than the minor axis, suggesting a prolate spheroidal shape. There is a subtle color gradient visible, with the central regions appearing more yellow/gold compared to the bluer outer regions. This color difference could indicate variations in stellar population, with older, redder stars concentrated towards the center and younger, bluer stars in the outer regions. No distinct spiral arm structures or dust lanes are discernible within the resolution of the image. The overall light profile appears relatively smooth, consistent with a relatively old stellar population and a low star formation rate. There is no indication of any major merger events or significant tidal disturbances.
