This galaxy appears to be a relatively smooth, elliptical or lenticular galaxy with a centrally concentrated bulge. The light profile appears somewhat diffuse and rounded, suggesting a lack of prominent spiral arms or distinct features. The core region exhibits a yellowish hue, potentially indicating an older stellar population. Moving outwards from the core, the color gradually shifts toward a bluer tint. The smooth morphology suggests a lack of ongoing major mergers, although there may be some minor gravitational interactions. Overall, the galaxy presents as a well-evolved system with a substantial mass and moderate levels of star formation.
