The galaxy appears to be a relatively smooth, elliptical system. There is no prominent disk structure visible, and the light distribution suggests a centrally concentrated bulge. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat elongated but not significantly cigar-shaped. There is no strong evidence of spiral arms or significant dust lanes. The color profile appears relatively uniform across the galaxy, with a suggestion of redder hues toward the center. No major merging events or tidal disturbances are readily apparent. Subtle features that could indicate minor disturbances or interactions cannot be entirely ruled out, but the overall morphology suggests a relatively relaxed and undisturbed system.
