The galaxy presents a largely smooth, elliptical morphology. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population and reduced star formation activity. The isophotes appear generally regular, with some minor irregularities in the outer regions. Fainter, diffuse extensions are barely perceptible, contributing to an overall sense of sphericity. The galaxy exhibits a significant concentration of light towards the center, and an overall moderate angular size. There are no readily identifiable spiral arms or dust lanes. The color gradient transitions from yellow in the core to a slightly redder color in the outer regions of the galaxy. The lack of blue light implies a paucity of young, massive stars.
