The galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a higher concentration of luminosity, gradually decreasing towards the outer edges. Its overall color profile suggests a dominance of older stellar populations, emitting predominantly in the redder wavelengths, but also shows some activity in bluer wavelengths. There may be some minor gravitational disturbances or interactions, as the shape isn't perfectly regular, and a faint tidal tail seems to be present. While it appears mostly isolated, there are potential signs of ongoing or recent merging events with smaller companions. It has a redshift consistent with cosmological expansion, indicating its significant distance from our vantage point.
