The galaxy presents as a relatively smooth, elongated structure. It exhibits a subtle color gradient, transitioning from a bluer hue at its outer edges to a slightly redder, brighter central region. The overall form is cigar-shaped rather than distinctly circular, suggesting a possible elliptical morphology. There are no obvious spiral arm structures or dust lanes visible. The galaxy's appearance is generally undisturbed, without evidence of ongoing major mergers, although slight irregularities in the light distribution hint at possible minor gravitational interactions or internal disturbances. Given the limited resolution, further classification requires more detailed spectral analysis.