The galaxy presents as an elongated, cigar-shaped structure. Its overall appearance is relatively smooth, with a soft, diffuse light distribution across the entire body. A slight color gradient is apparent, transitioning from a more yellow or golden hue near the core to a subtly bluer tinge in the outer regions. This suggests a possible difference in stellar populations, with the core potentially containing older, redder stars and the outer regions exhibiting some evidence of younger, bluer stars. There is no strong evidence of spiral arm structure or a distinct galactic disk. The overall impression is that this galaxy is in a relatively evolved state. Evidence suggests that this galaxy is not undergoing any major mergers, although minor disturbances cannot be ruled out.
