The galaxy presents an elliptical morphology, appearing largely smooth and well-defined. Its color profile suggests a relatively blue hue, potentially indicative of ongoing star formation. While the overall structure is smooth, there's a hint of disturbance or interaction visible on the periphery, suggesting a possible minor gravitational influence from a neighboring galaxy. The galaxy's core exhibits a strong central concentration, with brightness decreasing gradually toward the outer edges. A slight asymmetry is noted, but no definitive tidal features or prominent spiral arms are discernible. It appears largely undisturbed, but with a slight possibility of minor merging activity.
