The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution indicative of an older stellar population. The core exhibits a yellowish hue, possibly indicating a concentration of older, redder stars, or dust obscuration. Moving outwards from the core, the galaxy transitions to a bluer color, suggesting a component of younger, hotter stars, potentially within a disk structure viewed at an angle.

The overall shape is elongated, with an axial ratio suggesting it is not a perfect sphere. There is no clear evidence of spiral arms or significant dust lanes, but subtle asymmetries hint at possible past interactions or minor disturbances. Overall the galaxy appears relatively quiescent, without significant ongoing star formation.
