The galaxy appears to be an elliptical type, characterized by a smooth, diffuse light distribution, concentrated toward the center. The galaxy exhibits a roughly spheroidal shape, with only a slight deviation from perfect circularity. The color gradient shows a redder hue in the central bulge, transitioning to bluer colors in the outer regions. This suggests a central population of older, redder stars and the possibility of some younger, bluer stars in the surrounding areas. The lack of distinct spiral arms or a well-defined disk indicates that it lacks significant ongoing star formation. There are hints of a minor disturbance, possibly tidal features or faint asymmetries. The overall structure suggests a galaxy that has undergone significant evolution, possibly including past mergers.
