The galaxy presents as a flattened, elongated structure, appearing cigar-shaped when viewed from our perspective. The galaxy exhibits a relatively smooth, featureless morphology, with a dominant, centrally concentrated bulge. There is very faint suggestion of a disk component, but no obvious spiral arms. The galaxy displays colors that suggest a mix of stellar populations, with a slightly redder hue indicative of older stars. Its size suggests it is a relatively large system with an estimated mass above 10^10 solar masses. The relatively red color and smooth morphology, combined with its absolute magnitude, hints at low star formation and indicates that this is likely a passive or quiescent galaxy. There is no evidence of any major mergers or significant tidal disturbances, suggesting a relatively undisturbed evolutionary history.
