The galaxy presents a largely smooth morphology, exhibiting an elliptical-like structure with a dominant central bulge. The light distribution suggests a relatively high degree of concentration toward the core. Faint, diffuse extensions are tentatively observed emanating from the main body of the galaxy, indicating the presence of a stellar halo. The color profile demonstrates a redder hue in the core, transitioning to slightly bluer tones in the outer regions. This color gradient potentially suggests a difference in stellar populations with older stars more concentrated in the center and younger stars more prevalent in the outskirts. No prominent spiral arms or dust lanes are clearly discernible, which is consistent with the classification of an elliptical galaxy. There is slight evidence of minor gravitational disturbance or interaction with a very small amount of asymmetry.
