The galaxy presents as a relatively smooth, elongated structure. Its morphology appears to be largely spheroidal, with a high degree of central concentration. The light distribution suggests a lack of significant spiral arm features. The galaxy's color gradient indicates a potentially older stellar population, characterized by a yellowish-red hue dominant across the central regions, shifting towards a bluer hue at the periphery. There are minimal signs of ongoing star formation. No signs of major mergers or tidal disturbances are evident. The galaxy's shape is distinctly cigar-shaped, suggesting an elliptical morphology viewed from an oblique angle.
