The galaxy presents a largely smooth, elliptical morphology. The core exhibits a high concentration of light, appearing nearly spherical with a yellow-white hue, suggesting an older stellar population dominating the central region. Moving outward from the core, the light intensity diminishes gradually. The overall shape is somewhat elongated, but not exceedingly so. There is a possible faint, disturbed pattern, suggesting a small tidal interaction. The galaxy doesn't display defined spiral arms or distinct dust lanes, further supporting its classification as an elliptical type. The galaxy appears relatively isolated within its immediate field, lacking any immediately obvious major mergers. The color gradient implies ongoing star formation.
