The galaxy exhibits a generally smooth morphology, with a degree of apparent central concentration. The overall shape is moderately elliptical, trending towards a more elongated, cigar-like form. There is no clear evidence of strong spiral arm structure or a prominent central bulge. Subtle irregular features or minor disturbances might be present within the galactic disk, but these are not particularly pronounced. The color profile appears relatively uniform across the galaxy, with a moderate yellowish tint suggesting an older stellar population and a relatively low rate of ongoing star formation.
