This galaxy presents as a generally smooth, elliptical morphology. There is a distinct central bulge exhibiting a concentrated, yellowish hue, indicative of an older stellar population. Moving outwards from the core, the light profile decreases smoothly, with the color gradually shifting towards bluer tones, suggesting the presence of some younger stars in the outer regions. While no strong spiral arm structures or significant dust lanes are visible, a subtle irregularity in the outer isophotes hints at possible past minor interactions or disturbances. The overall roundness of the galaxy leans more towards an elliptical shape than a highly flattened disk. No signs of ongoing major merger activity are immediately apparent.
