This galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a centrally concentrated bulge. The light distribution suggests a high degree of symmetry, with no obvious spiral arm structure or prominent dust lanes visible. The galaxy displays a yellowish-red color, potentially indicative of an older stellar population and relatively low levels of ongoing star formation. The roundness of the galaxy also reinforces its identification as an elliptical galaxy. There are no visible signs of any major mergers happening to it currently, or any tidal disturbances. 
