The galaxy presents as an elongated, cigar-shaped structure. The central region displays a high degree of concentration, appearing smooth and featureless. A noticeable color gradient is observed, with the core exhibiting a distinct yellowish-orange hue, potentially indicative of an older stellar population. Fainter, bluer light appears at the edges of the structure, suggesting regions of younger stars. There may be some minor disturbance, but the galaxy appears mostly undisturbed. The overall morphology suggests a likely classification as an elliptical galaxy.
