The galaxy presents an elliptical morphology, appearing largely smooth with a concentrated central bulge. A slight elongation is noticeable, deviating minimally from a perfectly circular shape. The galaxy exhibits a radial color gradient, transitioning from a bluer hue in the central regions to a redder color in the outer parts. This color gradient likely indicates a decreasing population of young, hot stars with increasing distance from the core. There are no apparent spiral arm structures or distinct dust lanes visible. No signs of recent major merger events or tidal disturbances.
