The galaxy presents as a relatively smooth, elongated structure. Its color profile indicates a dominant yellowish-orange hue, suggestive of an older stellar population. The galaxy's shape is distinctly cigar-shaped, with a high degree of ellipticity. There is no clear evidence of spiral arms or a well-defined disk. No pronounced dust lanes are visible, and there do not seem to be any signs of major mergers or significant tidal disturbances affecting the system's morphology.
