The galaxy appears to be elliptical or lenticular in morphology, exhibiting a generally smooth light distribution without prominent spiral arms or a well-defined disk structure. The central region is brighter and more concentrated, suggestive of a galactic bulge. Color gradients are present, with the central region exhibiting a yellowish hue, potentially indicating an older stellar population. The outer regions appear slightly bluer, possibly hinting at younger stars or ongoing, albeit subdued, star formation. There may be some minor tidal disturbances indicating interaction or past mergers, however no strong signs of major interactions. Overall, the galaxy appears to be relatively isolated and in a state of quiescence. 
