The galaxy presents as a single, somewhat irregular object. The central region appears to be dominated by a bright, diffuse spheroid component, with a high degree of central concentration. There is evidence of a more extended disk-like structure surrounding this core. The galaxy exhibits a relatively smooth morphology with minimal signs of internal structure or spiral arms. The colour is predominantly consistent with an older stellar population.

There are indications of tidal features and a possible ongoing merger. There appears to be an additional, small bright object that appears to be in the final stages of merging with the galaxy. There also appears to be faint tidal streams of stellar material in the area surrounding the core and disk components.
