The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The color profile suggests an older stellar population, primarily exhibiting yellow-orange hues, with a potential for very low ongoing star formation. The overall shape leans towards an intermediate sphericity, neither perfectly round nor highly elongated. There's no prominent evidence of spiral arms, bars, or active galactic nuclei features visible in this image. The galaxy appears relatively isolated with no major signs of tidal disturbances or ongoing merger events.
