The galaxy appears as a relatively smooth, elliptical-shaped object. The light distribution is centrally concentrated, exhibiting a bright core that gradually fades toward the outer edges. There's a slight elongation, suggesting a deviation from perfect circularity. Color gradients are subtle, but a slightly redder hue is observed in the central region, possibly indicating an older stellar population. No distinct spiral arms or prominent dust lanes are discernible, reinforcing the smooth morphological classification. There is no apparent interaction or disturbance of other galactic bodies. Overall, the galaxy seems to be an early-type system, likely an elliptical or lenticular galaxy, with little evidence of recent star formation.
