The galaxy presents an intermediate morphology, displaying characteristics of both a smooth, possibly elliptical structure, and a feature, which may be a disk. It appears elongated, but leaning towards a more round shape. A subtle but noticeable asymmetry hints at a possible interaction or minor disturbance. The galaxy exhibits a blueish hue, suggesting active star formation. The estimated stellar mass for this galaxy is substantial, indicative of a large and evolved system. Its inferred star formation rate suggests that stars are being born at a moderate rate, implying that it is no longer undergoing a major burst of star formation, nor is it quiescent.