The galaxy presents as a centrally concentrated object with an elliptical morphology. The light distribution appears relatively smooth with a dominant bulge component and faint, diffuse arms. It exhibits a gradual color gradient, transitioning from a yellowish-white core to slightly redder hues in the outer regions. There appears to be some mild distortion in the disk, along with a possible minor interaction with a smaller nearby body. The overall impression is of a mature galaxy with ongoing, but diminished, star formation activity.
