The galaxy presents a generally smooth, elongated morphology. Its overall shape is cigar-like, exhibiting a significant departure from circularity. The light distribution is relatively uniform, with no obvious spiral arm structures or strong central bulge. The galaxy exhibits a color gradient, trending from a more blue-ish white color at its edges to a more reddish gold hue at its center, indicative of varying stellar populations. The absence of prominent dust lanes or knots suggests a lack of ongoing, intense star formation. Minor disturbances possibly indicating a subtle interaction, appear to be present, but it is difficult to determine the nature of the interaction with certainty. The galaxy's size suggests it is a relatively large system.
