The galaxy appears as a centrally concentrated object with a smooth morphology. The shape is elongated, resembling a cigar-like structure, suggesting it is either an elliptical galaxy or a disk galaxy viewed at a high inclination. The galaxy exhibits a color gradient, appearing yellower and more concentrated toward the center, indicating an older stellar population. There are no prominent spiral arms or dust lanes visible, supporting the interpretation of a smooth, potentially elliptical morphology. There is no evidence of any merging or tidal disturbances; the galaxy appears relatively undisturbed.
