The observed galaxy exhibits a generally smooth morphology, with a noticeable elongation along its major axis. Its overall form suggests a transition between elliptical and lenticular types. The central region displays a higher concentration of light, appearing more uniform and slightly redder in color, indicative of an older stellar population. The outer regions show subtle color gradients, with faint bluish tints potentially indicating the presence of younger stars. Possible minor disturbances in the morphology on one side of the galaxy suggest a possible interaction with a nearby galaxy. The main body of the galaxy does not seem to have strong spiral arms or significant dust lanes. Overall the galaxy appears to be relatively quiescent.
