This galaxy appears to be a relatively smooth, centrally concentrated object. Its light profile exhibits a high degree of radial symmetry with a round shape. There is a slight color gradient, transitioning from slightly bluer hues in the central region to redder tones in the outskirts. There are no prominent spiral arms, bar structures, or tidal features visible suggesting it is unlikely to be undergoing any major merging or disturbance. The overall color suggests a population of older stars, with ongoing star formation at a reduced rate. Given the redder outer colors, this also indicates that the outer regions are composed of older stars. The galaxy appears to be a fairly massive system. 
