The galaxy presents a concentrated central bulge, appearing bright and relatively smooth. Surrounding the core is a faint disk component, with some indication of disturbed morphology. The disk is slightly asymmetric, hinting at possible interactions or recent mergers. Overall, the galaxy appears to be in a transitional state, showing characteristics of both elliptical and spiral galaxies, with a possible interaction or merger. The colour index suggests a population of both young and old stars, with some regions displaying a bluer hue and some areas appear to have a redder hue.
