The galaxy presents a distinctly elongated, cigar-shaped morphology. Its color is primarily a muted bluish-white, suggesting the presence of a moderate population of young, hot stars, but also significant older stellar populations. The light distribution appears relatively smooth with a slight concentration towards the center, lacking any prominent spiral arms or strong dust lanes. There is no clear central bulge. Faint hints of irregularities or minor disturbances in its structure are potentially visible at the edges, though these could be artifacts. Based on the moderate blue color, the galaxy seems to show hints of star formation, albeit at a relatively low rate. No signs of ongoing major merger activity are seen.
