The galaxy presents a primarily smooth morphology, with an elliptical shape and a high degree of central concentration. Its overall form appears to be somewhere in between round and elongated, with no obvious signs of a distinct disk. The luminosity profile suggests a relatively uniform stellar population with very little evidence of ongoing major star formation. There may be a faint indication of a minor tidal disturbance or possible interaction, but the dominant impression is of a relaxed system. The object appears to be relatively isolated with no other large galaxies in close proximity.
