The galaxy presents a generally smooth, elliptical morphology. It appears largely spheroidal in shape, exhibiting a high degree of roundness with minimal discernible disk-like features or spiral arms. There is no strong indication of active galactic nuclei or a bright central point source. The galaxy demonstrates a subtle color gradient, appearing somewhat bluer in its core region, trending to redder hues further from the center. We can detect a slight deviation in the general morphology indicating it may be undergoing minor disturbances and or a small merger. The stellar population is likely dominated by older stars with a lower rate of ongoing star formation, suggested by the subtle color change between the core and more distanced stellar populations. 
