The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with a concentration of light towards the center, suggesting a prominent bulge. The primary body of the galaxy displays a color gradient transitioning from a yellow-orange core to a faint blue-green towards what appears to be one edge. This color variation may indicate differential stellar populations or dust obscuration. There is a subtle distortion or asymmetry observed within the blue-green region, possibly a minor disturbance. Overall the galaxy appears slightly elongated, with the major axis moderately exceeding the minor axis. The galaxy's structure appears relatively unperturbed, and there does not seem to be evidence of an ongoing major merger.
