The galaxy presents as a somewhat elongated structure, appearing more cigar-shaped than perfectly circular. Its overall appearance is relatively smooth, with a lack of prominent spiral arms or distinct features. There is a subtle color gradient, with a slightly bluer hue visible towards one end, possibly indicating a region of ongoing or recent star formation. The central region exhibits a concentration of light, suggesting the presence of a galactic bulge. There are hints of minor disturbances or asymmetries in the galaxy's morphology, potentially indicating past interactions or mergers, though no major merging events are immediately apparent. Overall, the galaxy seems to be a relatively massive system with a low specific star formation rate.
