The galaxy presents as a concentrated, elliptical-like structure with a smooth appearance. Its color profile is dominated by reddish hues, suggesting an older stellar population with limited ongoing star formation. The galaxy exhibits a high degree of central concentration, with luminosity decreasing smoothly from the core outwards. It demonstrates a moderate degree of ellipticity. There is no clear evidence of spiral arms or prominent dust lanes. The overall morphology is relatively undisturbed, and no major mergers or tidal features are readily apparent.
