The galaxy presents an elongated, cigar-shaped morphology. Its light appears relatively smooth and concentrated towards the center, suggesting a dominant bulge component. The color is primarily blue-white, hinting at the presence of a population of relatively young, hot stars. There is no apparent spiral structure or evidence of significant dust lanes. The galaxy appears undisturbed, with no visible signs of tidal tails or other features indicating a recent major merger event. Given the smooth light distribution and elongated shape, this galaxy is likely an elliptical or lenticular galaxy.
