The galaxy appears to be a relatively compact system, possibly elliptical or lenticular in nature. The light profile seems smooth, lacking prominent spiral arms or strong, irregular features. There is a noticeable color gradient, with a brighter, bluer central region transitioning to a yellower, dimmer outer halo. This could suggest recent star formation concentrated in the core, while the outer regions are populated by older stellar populations. There may be a hint of tidal disturbance or a minor companion galaxy in close proximity, given its shape. The galaxy is moderately luminous and likely possesses a substantial stellar mass. Based on color indices, star formation is most likely supressed.