The galaxy appears to be a relatively smooth, spheroidal object, exhibiting a high degree of circular symmetry. There is a concentrated central region that transitions gradually into an extended halo. The color profile indicates an older stellar population, showing predominantly yellow and red hues. There are no apparent spiral arms or distinct dust lanes visible in the image. The galaxy seems undisturbed, with no indications of major mergers or tidal interactions, although there may be some minor disturbances. It is considered a massive galaxy with very little ongoing star formation.
