The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. The light profile appears diffuse, with a gradual decline in intensity from the core outwards. There is a slight elongation; however, the galaxy appears mostly circular. Color gradients are subtle; the central region exhibits a slightly redder hue compared to the outer regions, which appear more blue/green. The light distribution suggests a relatively evolved stellar population, although some ongoing star formation cannot be ruled out based on the bluer outer colors. There is no readily discernible evidence of spiral arms, bars, or significant dust lanes. Tidal features are absent, suggesting no recent major merger events. The galaxy shows only a very minor disturbance, with a smooth and rounded shape, but may be undergoing a minor merging event. Overall, the galaxy presents as an elliptical or lenticular type galaxy.
