The galaxy presents a largely smooth, elliptical morphology with minimal visible substructure. It exhibits a centrally concentrated luminosity profile, indicative of a prominent bulge. The color appears predominantly blue-white in the central regions, suggesting the presence of a population of relatively young, hot stars. A slight radial color gradient is perceptible, with the outer regions appearing somewhat redder than the core, which could indicate an older stellar population in the outskirts. There is no clear evidence of spiral arms, bars, or significant dust lanes. The overall shape is close to circular, showing minimal signs of elongation or tidal disturbances. There is no immediate evidence of a major ongoing merger, although some slight asymmetry cannot be ruled out.
