The galaxy presents an elongated, cigar-shaped morphology. There appears to be a relatively smooth, central bulge exhibiting a yellowish-orange hue, suggesting a population of older stars. Extending outwards from the bulge, a faint disk structure is visible, displaying a bluer color, indicative of younger stars and possible ongoing star formation. The disk structure is not well defined and appears somewhat disturbed or irregular. No prominent spiral arms or bar features are discernible in the image. There might be some evidence of minor tidal disturbance or interaction, but the overall structure suggests it is not currently undergoing a major merger event.
