The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated light profile. A bright, yellowish core region transitions into a bluer, more diffuse outer halo. The overall shape is elongated, suggesting a non-spherical distribution of stars within the galaxy. There is no clear evidence of spiral arm structures or significant dust lanes. Subtle irregularities in the outer regions may indicate minor disturbances or interactions, but the overall structure appears largely undisturbed. Color gradients suggest a stellar population gradient, with older, redder stars concentrated towards the core and younger, bluer stars more prevalent in the outer regions. Star formation is present at a low level. The galaxy displays a stellar mass that qualifies it as a massive galaxy.
