The galaxy appears to be a relatively compact system with a notable central bulge. The light profile suggests a generally smooth distribution, though there is some evidence of asymmetry in the outer regions. The color gradient indicates a redder core, possibly due to an older stellar population, transitioning to bluer hues in the outer disk. The suggestion of a disk is present, with a slight flattening of the galactic structure. There is some evidence of minor disturbances or interactions, though no major ongoing merger events are clearly visible. The galaxy does not appear perfectly circular and is somewhere in between round and cigar shaped.
