The galaxy presents as a relatively compact, elliptical system. Its central region exhibits a high degree of smoothness, with light distribution suggesting a bulge-dominated morphology. The overall color appears to be trending towards redder hues, indicative of an older stellar population and diminished ongoing star formation. While no distinct spiral arms or disk structures are clearly discernible, the isophotes show a slight deviation from perfect circularity. There is some indication of possible tidal disturbances or minor asymmetries in the outer halo region.