The galaxy presents as an elongated, cigar-shaped structure. Its overall morphology appears relatively smooth with a high degree of central concentration in a yellowish hue, hinting at an older stellar population in the core. The outer regions of the galaxy display a faint, bluer tinge. This color gradient from core to periphery could indicate a difference in stellar population ages, with younger, bluer stars residing in the outer regions. There is little evidence of prominent spiral arms or significant dust lanes. The galaxy exhibits a small perturbation, but is most likely undisturbed.
