The galaxy presents a somewhat amorphous structure, appearing neither definitively elliptical nor spiral. It shows a central region of moderate brightness, with a slightly elongated profile.

The color distribution is not uniform. The central region appears to exhibit a bluer hue, possibly indicating the presence of younger stellar populations or active star formation. Fainter, diffuse extensions are visible, displaying a slightly redder color suggesting older stars.

Some irregular features or disturbances are present, potentially indicative of tidal interactions or past merger events. There also seems to be some indication of some tidal tails and distortions.

The galaxy's overall form suggests it may be in a transitional stage, potentially evolving from a disk-dominated system into a more spheroidal shape.
