The galaxy presents as a smooth, elongated, cigar-shaped object. The galaxy exhibits a noticeable central bulge which appears bright yellow, with the luminosity fading gradually towards the edges. There appears to be little or no spiral structure visible. The overall color index suggests a population of older stars. No major mergers or significant tidal disturbances are apparent, with only slight indications of minor disturbances, likely indicative of relative gravitational stability. The galaxy exhibits a moderate redshift, suggesting a considerable distance from the observer. The half-light radius is significant, indicating it is a fairly large galaxy. The lack of distinct blue regions suggests a low ongoing star formation rate.
