The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in texture, with a concentration of light towards the center. The color distribution suggests a dominant population of older stars, as indicated by the reddish-yellow hue of the central region. Some bluer tints suggest the presence of younger star formations in the outer regions. There is no clear evidence of a spiral arm structure or bar. The overall appearance suggests a galaxy that is potentially an elliptical type. There are no obvious signs of major disturbances or ongoing mergers.
