The galaxy appears as a centrally concentrated object with a somewhat diffuse morphology. The light distribution suggests a smooth profile, with no readily discernible spiral arms or bar structure. There is a slight elongation observed, though the overall shape appears approximately elliptical. The galaxy's color profile displays a slight reddish hue, particularly towards the center. No strong tidal features or signs of major merger activity are evident. Subtle irregularities in the outer regions may indicate minor disturbances, but these features are not highly pronounced. Overall, the morphology suggests a galaxy likely undergoing passive evolution, possibly an elliptical or lenticular type.
