The galaxy exhibits a generally smooth morphology, lacking any prominent spiral arms or a well-defined disk structure. It is a centrally concentrated object with a roughly elliptical shape, with the core region displaying a bright yellowish hue, suggesting the presence of older stellar populations and possibly a supermassive black hole actively accreting material. The galaxy appears relatively isolated, showing no significant signs of ongoing or recent major mergers. There might be a subtle suggestion of minor disturbances in the outer regions of the galaxy. Overall, the galaxy seems to be relatively evolved with limited ongoing star formation activity.