The galaxy presents as a relatively compact object, with a smooth, elliptical-like morphology, indicative of a spheroid-dominated system. Its overall color profile suggests a mature stellar population, with a concentration of older stars toward the central regions. This is supported by the yellowish-orange hue observed in the galaxy's core, contrasting with the slightly bluer outskirts. The luminosity profile appears centrally concentrated, fading smoothly towards the edges. There is subtle evidence of possible tidal features or minor disturbances in the outer regions of the galaxy, implying past or ongoing gravitational interactions, although no clear signs of ongoing merging. Some areas of star formation appear to be occurring, as evidenced by small red areas surrounding the central spheroid.
