The galaxy presents as a relatively smooth, elliptical structure. There is a concentration of light towards the center, indicating a prominent bulge. The light profile appears to fade gradually from the core to the outer regions. There are no obvious spiral arm structures visible, nor are there any clear signs of major disturbances or ongoing mergers. The color appears to be somewhat redder overall, especially in the central bulge, suggesting an older stellar population. There is little evidence of significant ongoing star formation activity based on the lack of blue light concentration. The overall shape is somewhat rounded, exhibiting a moderate ellipticity.
