The galaxy presents as an elliptical morphology, with a high degree of central concentration and a smooth, diffuse light profile. The core appears bright and yellow, indicative of an older stellar population dominating the central region. The isophotes are generally elliptical and concentric, showing a moderate ellipticity that is slightly deviating from circular. There is little evidence of spiral arm structures or distinct features such as dust lanes or star-forming regions. The galaxy exhibits a color gradient, with the outer regions appearing slightly redder, which potentially suggests a decreasing age of stellar populations from the core outwards. No obvious signs of tidal disturbances or recent merger activity are observed, suggesting a relatively undisturbed evolutionary history. Overall, the galaxy appears to be a fairly massive, evolved system with ongoing, but comparatively low, levels of star formation.
