The galaxy presents as a smooth, elliptical morphology, appearing largely featureless. Its overall shape is noticeably elongated, more akin to an ellipse than a perfect circle. The central bulge is prominent and exhibits a concentrated luminosity, suggesting a high density of stars within that region. The color gradient transitions smoothly from a yellowish core to a redder outer halo. This color variation may indicate differences in stellar populations and age, with the core potentially dominated by older, redder stars. There is a subtle hint of a disk-like structure but lacks defined spiral arms or distinct dust lanes. There is no evidence of major merging events or significant tidal disturbances, and the galaxy appears relatively undisturbed.
