The galaxy presents an overall elliptical morphology, appearing elongated with a cigar-like shape. The central region exhibits a higher surface brightness, suggesting a dense stellar population likely associated with a galactic bulge. The light distribution appears smooth, without prominent spiral arms or significant dust lanes visible in this image. Color gradients are observed within the galaxy. The core appears to be a yellow hue, which could indicate an older stellar population or the presence of dust. Progressing outwards, the galaxy becomes more bluish in color. It may also be experiencing some minor disturbance.