The galaxy exhibits a generally smooth morphology, appearing largely featureless at this resolution. Its shape is approximately round, though not perfectly circular, possessing a moderate ellipticity. There is no strong evidence of spiral arm structure or a prominent central bar. The color profile indicates a redder hue, suggesting a population of older stars and potentially a lower rate of on-going star formation within the galaxy. There is no visually apparent sign of tidal disturbances or ongoing merger activity; the galaxy appears relatively undisturbed in its morphology.
