The galaxy exhibits an elongated, cigar-shaped morphology. Its light profile appears relatively smooth, with no distinct spiral arms or a prominent central bulge visible at this resolution. The color gradient indicates a higher concentration of bluer light towards the central regions, potentially suggestive of ongoing star formation or a younger stellar population. There is some hint of dust lanes or substructure that could contribute to the observed form. There are no significant signs of major disturbances or tidal features.
