The galaxy presents as a diffuse, ellipsoidal object with a reddish-yellow hue. There is evidence of a central concentration of luminosity, suggesting a possible core or bulge. The outer regions of the galaxy appear less defined, fading gradually into the background. There seems to be a companion object or tidal debris located nearby, possibly indicating an interaction or past merger event. The overall structure is relatively smooth, with no clear spiral arm features or distinct dust lanes discernible at this resolution. The morphology appears more characteristic of an elliptical galaxy with a moderate amount of internal disturbance or ongoing interaction. The galaxy’s color suggests an older stellar population.
