The galaxy presents a moderately smooth, elliptical morphology. It exhibits a prominent central bulge, which appears nearly spherical and is characterized by a bright, concentrated luminosity. A disk component, while present, is less defined, showing a flattened structure surrounding the bulge. The overall color profile indicates a mix of stellar populations, with the central region appearing slightly yellower, suggesting older, redder stars, while the outer disk shows hints of bluer tones, possibly indicating more recent star formation activity. There is a subtle asymmetry visible, potentially indicative of a minor gravitational interaction or internal disturbance. There is no clear evidence of a recent major merger; however, subtle irregularities and a disturbed appearance suggest a system that might be experiencing a minor interaction or a post-merger phase. A very slight tidal tail or plume might be extending from the galaxy, although it blends in with the surrounding background.
