The galaxy presents a predominantly smooth morphology, suggesting it may be an elliptical or lenticular type. There is a hint of a disk or possibly a spiral structure but it is not distinct. The core region exhibits a higher luminosity, possibly indicating a concentration of older stellar populations. The galaxy's color profile appears slightly redder in the central regions, shifting towards bluer tones in the outer edges, which could indicate recent or ongoing star formation further from the core. There is a suggestion of minor gravitational disturbance or interaction occurring, though a definitive merger is not immediately apparent. The shape of the galaxy is somewhere between round and cigar-shaped.
