The galaxy presents as a relatively small, elongated system. Its morphology appears largely smooth and featureless, lacking prominent spiral arms or distinct substructures. The galaxy exhibits a color gradient, with a slightly bluer central region transitioning to redder hues towards the edges, possibly indicating differential stellar populations or dust content. The shape is significantly elongated and somewhat irregular, more akin to a cigar shape. There is no clear evidence of on-going major mergers or significant tidal disturbances. The overall appearance suggests that it is a late-stage galaxy that has exhausted much of its gas supply and has a low star formation rate.
