The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, appearing moderately elongated rather than perfectly spherical. The color profile indicates a redder central bulge, transitioning to slightly bluer hues in the outer regions, suggesting a differential stellar population distribution. There is no clear evidence of prominent spiral arm structures or ongoing major merger activity. Subtle distortions in the outer envelope may indicate minor tidal interactions or past disturbances, but these are not overwhelmingly pronounced. The galaxy's overall appearance suggests a system with a relatively low star formation rate, consistent with a more evolved stellar population.
