The galaxy appears to be a relatively compact system, exhibiting a largely smooth morphology with hints of more complex structure within. The light profile suggests a centrally concentrated bulge component. Overall, the galaxy presents a primarily elliptical shape. There seems to be some slight asymmetry, potentially indicating minor gravitational disturbance. Color gradients are subtle, with a possible concentration of slightly bluer light in the central regions, indicative of ongoing star formation. The outer regions appear redder in comparison. No distinct spiral arms or prominent dust lanes are visible, but subtle deviations in the surface brightness and color could be indicative of recent or ongoing merger activity.
