The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. It exhibits a nearly circular profile, suggesting a minimal degree of apparent ellipticity. The galaxy's light is dominated by a reddish hue, with some evidence of bluer emissions in its center, which may hint at a small amount of recent star formation activity in the core region. The overall structure appears undisturbed, lacking obvious signs of tidal tails or major merger activity. It seems to be a relatively isolated system.
