The galaxy appears as a moderately bright, elongated object, exhibiting a relatively smooth morphology. The light distribution suggests a central concentration, with a radial decrease in intensity outwards. The shape can be described as somewhat cigar-shaped, and there is minimal evidence of spiral arm structure or significant dust lanes. Its overall color appears to be somewhat redder, which could be caused by older stellar populations. There is a faint suggestion of minor tidal disturbances or interactions occurring, with a faint extension on one side of the galaxy. Overall, the galaxy's appearance suggests a lack of recent major mergers or significant star formation activity, and it appears to have a substantial mass.
