The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish in color, suggesting an older stellar population. The galaxy displays a gradual decrease in surface brightness moving outward from the center, with a faint, diffuse halo extending beyond the core. No obvious spiral arm structure or dust lanes are apparent. There may be some signs of minor tidal disturbances in the outskirts, although this requires further verification with higher resolution data. The overall morphology indicates a galaxy that is likely undergoing minimal current star formation.
