The galaxy presents as an elongated, diffuse object. The light distribution appears relatively smooth and centrally concentrated. The color profile shifts from a bluer hue at the edges to a redder hue towards the center. This suggests a difference in stellar populations or dust content between the outer regions and the nucleus. There's a subtle asymmetry in the galaxy's shape that may indicate a minor gravitational disturbance or ongoing interaction, though a merger event is not readily apparent. Overall, the galaxy appears to be an elliptical or lenticular galaxy exhibiting a degree of redshifting.
