The galaxy presents as a largely smooth structure, with a notable absence of well-defined spiral arms or a prominent central bar. It appears elongated, exhibiting a cigar-like shape rather than a perfectly circular disk. The light is centrally concentrated, showing a gradual decrease in intensity towards the outer edges. There is subtle color variation across the galaxy, with a suggestion of bluer hues in the outer regions and a slightly redder or yellower tone towards the core, hinting at variations in stellar populations or dust distribution. No significant signs of ongoing major merger activity, although the slight irregularities in the outer contours could suggest minor disturbances. The overall morphology is consistent with a galaxy transitioning towards a more spheroidal or elliptical form.
