The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth morphology without prominent spiral arms or a well-defined disk structure. It has a fairly round shape, with only minor deviations from circular symmetry. The central region is bright and relatively homogenous in color, likely indicating an older stellar population. There is some indication of a slight disturbance in the galaxy's structure, possibly from a minor interaction with another galaxy, but is not considered an actively merging system. Overall, the galaxy seems to be relatively quiescent, with a low star formation rate.
