The galaxy presents a somewhat disturbed morphology, potentially indicative of an ongoing or recent interaction. A significant portion of its light appears concentrated within a central, relatively smooth component, but there's also evidence of fainter, more diffuse emission extending outwards. The galaxy exhibits a yellow hue, suggesting a population of older stars. It appears to be undergoing star formation at a relatively low rate. A possible minor merger can be seen as a secondary bulge-like feature above the main body of the galaxy.