The galaxy presents an elongated, cigar-like morphology. The central bulge appears relatively prominent and exhibits a yellowish hue, suggesting a population of older stars. The disk component is less defined, showing a smoother appearance and bluer colors towards the outer regions, which could indicate ongoing star formation. There is no clear evidence of spiral arm structure or a well-defined disk. Overall, the galaxy exhibits a smooth, undisturbed appearance with only minor asymmetries, hinting that it is not undergoing major merger activity.
