The galaxy presents as a relatively smooth, elongated structure. It exhibits a generally featureless morphology, with a somewhat cigar-shaped appearance. A subtle color gradient is visible, transitioning from a bluer hue in the central region to slightly redder tones towards the outer edges. This color variation potentially indicates differences in stellar populations, with younger, hotter stars concentrated toward the core and older, cooler stars populating the outskirts. There's no apparent spiral arm structure, bar, or other distinct morphological features. The galaxy shows no signs of any major merger events.
