The galaxy presents an elliptical morphology, exhibiting a relatively smooth light distribution. The central bulge region is bright and concentrated, with a yellow-white hue, potentially indicative of an older stellar population.  Moving outwards from the core, the luminosity decreases gradually, with a subtle transition in color towards a slightly bluer periphery, suggesting the presence of some younger stars or ongoing, albeit limited, star formation in the outer regions. While the galaxy appears largely undisturbed, there is a hint of minor asymmetry or a possible faint tidal feature on one side, meriting further investigation into potential past interactions. The galaxy's overall shape is moderately elongated, but not excessively so.
