The galaxy presents as an elliptical morphology, exhibiting a generally smooth appearance. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. There is a slight elongation in its shape but a general roundness. The galaxy's color appears yellowish-orange, implying an older stellar population, with minimal presence of dust. No distinct spiral arms, bar structures, or signs of recent star formation activity are apparent. There are no obvious signs of tidal tails or distortions, suggesting it is not undergoing a major merger. The overall structure suggests that the galaxy is a relaxed system, having undergone significant evolutionary processes.
