The galaxy presents a generally smooth morphology, displaying a centrally concentrated brightness profile. It appears largely elliptical, though not perfectly spherical. The core region exhibits a distinct red hue, possibly indicative of older stellar populations or dust obscuration. Surrounding this core is a more diffuse, greenish halo. The green color may suggest the presence of some ongoing star formation, although not at a prodigious rate. There is no strong evidence of spiral arm structures or significant tidal disturbances. Overall, the galaxy appears to be relatively isolated and undisturbed, characteristic of a more evolved system.
