The galaxy appears to be a relatively smooth and rounded elliptical galaxy, exhibiting a somewhat uniform color gradient that transitions subtly from a brighter center to a slightly dimmer, less defined edge. There is no apparent dust lane, spiral arm structure, or bar. The overall structure suggests an older stellar population, lacking significant ongoing star formation. There is no sign of any active galactic nucleus or a substantial amount of ionized gas, evidenced by the lack of bright blue or pinkish regions typically associated with star forming nebulae. There are no features that indicate it is currently undergoing a major merger, although the presence of subtle disturbances within the galaxy cannot be entirely ruled out.
