The galaxy appears as a relatively smooth, centrally concentrated object, exhibiting a slightly elliptical morphology. The light distribution suggests a dominant bulge component, with a gradual decrease in intensity outwards from the core. Faint wisps of diffuse light extend outwards from the main body, potentially indicating tidal interactions or recent merger activity. The galaxy's color profile suggests a population of older stars, with the core potentially hosting a more actively star-forming region as suggested by the green hue. Overall, the galaxy appears to be in a state of ongoing evolution, characterized by a combination of quiescent stellar populations and hints of recent or ongoing interactions. 
