The galaxy appears as a flattened, elongated structure with a smooth overall profile. The light distribution suggests a concentration of older stellar populations, and the galaxy's shape hints at an elliptical morphology. There is no apparent evidence of spiral arms or significant dust lanes. The galaxy exhibits a slightly redder color, indicating a lower rate of ongoing star formation and a dominance of older, redder stars. There is no evidence of active galactic nuclei activity or significant tidal disturbances, suggesting the galaxy is relatively isolated and undisturbed. The shape of the galaxy tends towards a cigar-like form, with an intermediate thickness. Based on these characteristics, the galaxy is most likely an elliptical galaxy with little or no current star formation.
