The galaxy presents a clear spiral morphology. Two distinct spiral arms are visible, emanating from a moderately sized central bulge. The arms exhibit a relatively tight winding pattern. The overall color suggests ongoing star formation, with a bluer hue in the arms indicating the presence of younger, hotter stars, contrasting with the yellower central bulge which may indicate older stellar populations. There's no obvious bar structure bisecting the central region. There is no sign of tidal disruption or other major disturbances, implying it is not currently undergoing a major merger event. The galaxy is neither a pure elliptical nor a pure disk galaxy, possessing components of both morphologies.
