The galaxy presents as a primarily smooth, rounded object with some evidence of potential interactions or disturbances in its morphology. The galaxy is redshifted to a value of 0.340509, which indicates that it is relatively distant. The overall structure appears amorphous, lacking distinct spiral arms or a well-defined bar structure.

The central region exhibits a high concentration of light, suggestive of a prominent galactic bulge. The color profile of the galaxy indicates a greater concentration of redder light in its central regions, possibly indicating an older stellar population. Fainter, bluer light is faintly visible in the outer regions. The galaxy has an estimated effective radius of approximately 12 kpc. The color indices suggest a stellar mass estimate of 10^11.4 solar masses. Star formation rate is very low.

There is a possible merging event occuring with this galaxy.

