The galaxy presents as a centrally concentrated system, appearing largely featureless and smooth. It exhibits a generally elliptical morphology, with a high degree of roundness. The color profile suggests an older stellar population dominating the light output, trending towards redder wavelengths in the central region and fainter, somewhat bluer wavelengths on the edge. There is no readily apparent evidence of spiral arm structure, a prominent disk component, or major ongoing merger activity. Minor disturbances may be present but are not immediately obvious. The galaxy exhibits a significant luminosity, with an estimated size of approximately 9.5 kpc, suggesting it is a massive system. There is no obvious evidence of intense star formation. The color, morphology, and lack of defined structure suggest it is a passive galaxy.
