The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth morphology with minimal discernible features. The light distribution is concentrated towards the center, indicating a high stellar density in the core. The overall shape appears predominantly round, lacking any significant elongation or bar structure. There is no evidence of major ongoing mergers or significant tidal disturbances affecting the galaxy's structure. The outer regions of the galaxy are more diffuse, suggesting a gradual decrease in stellar population density moving away from the galactic center. Color gradients are subtle; the core appears slightly yellower, potentially indicating an older stellar population, while the outer regions are marginally bluer, possibly hinting at some level of recent or ongoing star formation, though this activity is not pronounced.
