The galaxy presents a somewhat disturbed morphology, potentially indicative of an ongoing or recent interaction or merger event. The central region exhibits a high degree of sphericity with a smooth texture, suggesting a significant population of older stars. There is a possible tidal tail or bridge of material extending from the galaxy, displaying a more irregular and less-defined structure. The colors suggest a range of stellar populations, with the central region appearing more yellowish, indicative of older stars, and the outer regions having a slight blue tinge, suggesting the presence of younger, hotter stars and possibly some star formation activity. The overall appearance is not a perfectly symmetric elliptical or spiral, hinting at dynamical processes influencing the observed morphology. There appears to be a second, smaller object in close proximity that may be interacting with the larger galaxy.
