The galaxy appears to be an elliptical or lenticular type, exhibiting a largely spheroidal morphology with a smooth, diffuse light distribution and a prominent central bulge. There is no apparent spiral arm structure or significant dust lane obscuration. The core appears to be yellowish, possibly indicating a population of older stars, and a lack of significant recent star formation activity. The outer regions are more blueish in color, suggesting younger stars. The overall structure is relatively undisturbed, showing no signs of major mergers or tidal interactions with other galaxies. The overall form appears round. There are no clearly discernible features suggesting active star formation, such as HII regions. The gradient in color from the center to the outer regions may be due to variations in stellar populations.
