The galaxy presents as a relatively smooth, roundish object with a bright central bulge. There is little evidence of spiral arm structure or significant dust lanes. The color appears primarily blue-white, suggesting a population of relatively young, hot stars. The overall morphology is consistent with an elliptical galaxy, though a very subtle flattened disk-like component cannot be entirely ruled out. There are no obvious signs of recent major merger activity or tidal disturbances. The galaxy exhibits a fairly concentrated luminosity profile, with the majority of its light emanating from the core region. It displays a hint of a yellowish-red hue in the central bulge.
