The galaxy presents as an elongated, cigar-shaped structure with a smooth, diffuse appearance. The central region exhibits a slightly brighter and more concentrated luminosity, suggesting a possible galactic bulge. The overall color profile indicates a mixture of stellar populations, with a subtle gradient from a possibly redder core to slightly bluer outer regions. There is no apparent spiral arm structure or distinct dust lanes visible, and it lacks any strong tidal features or signs of recent major mergers. The galaxy exhibits a relatively low rate of star formation.
