The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, indicative of an older stellar population. A slight color gradient is perceptible, with the central region exhibiting a warmer, yellower hue that transitions to cooler, bluer tones towards the outer edges. This suggests a potential difference in stellar age or metallicity between the galactic nucleus and the outskirts. The galaxy is mostly spheroidal, with minimal discernible features of spiral arms or a defined disk. There is no clear evidence of tidal disturbances, indicating the system is relatively undisturbed, possibly in a quiescent state.
