The galaxy presents as a single, relatively smooth object with no prominent spiral arm structure or bar apparent. The overall morphology is elliptical or lenticular. Color gradients within the galaxy suggest a centrally concentrated stellar population with a yellowish hue, potentially indicating older stars. The galaxy appears moderately compact, and with a faint halo or extended emission around the central region. There is very little evidence of dust lanes or active star formation, the system appears quiescent. The shape is mostly round. There are no signs of tidal tails or ongoing mergers, but subtle asymmetry indicates possible past interactions or disturbances.
