The galaxy presents a predominantly smooth morphology. Its shape is noticeably elliptical, tending towards a more rounded form rather than a highly elongated or cigar-like appearance.  A central bulge region is visible, exhibiting a yellowish hue, suggesting an older stellar population. Fainter, diffuse light extends outwards from the core, showing a slight change in color to redder tones in the outer regions, potentially indicating a presence of dust and slightly older stars away from the galactic center. The disk exhibits no obvious spiral arm structures.  There are slight indications of minor disturbances within the galaxy structure. No significant signs of ongoing major merger events are readily apparent.
