The galaxy presents as a somewhat amorphous, elliptical structure. It exhibits a smooth, diffuse appearance with no distinct spiral arms or a defined central bulge. The color is generally a uniform hue, suggesting a relatively old stellar population with ongoing star formation. The galaxy's shape is elongated, tending toward a cigar-like form. No apparent signs of major mergers or tidal disturbances are observed, although subtle indications of minor interactions or internal restructuring cannot be ruled out at this resolution.
