The galaxy appears as a relatively smooth, elliptical object with a bright central bulge. The light is dominated by yellow and red wavelengths, suggesting an older stellar population. There is some indication of a faint disc with subtle bluer regions hinting at the presence of younger stars, but it is not well-defined. A small, diffuse region of enhanced red emission is visible to the left of the galaxy's core, possibly a region of recent star formation or a tidal feature. The overall shape is generally rounded, but with a slight asymmetry, which could be indicative of a minor interaction. The galaxy does not appear to be undergoing a major merger, but subtle disturbances might be present.
