The galaxy presents an elongated, cigar-shaped morphology. The primary structure exhibits a smooth distribution of light, with a slight concentration towards a central region. There is a noticeable color gradient, transitioning from cooler, redder hues at the lower end of the galaxy to a bluer tint at the opposite end. Evidence of minor disturbances is present within the galaxy's structure. The observed smoothness suggests a later-type galaxy, although the elongated shape indicates a possible ongoing interaction or tidal distortion event. Overall the galaxy appears to be fairly isolated in its environment.
