This galaxy appears to be a relatively smooth, elliptical galaxy. The light profile indicates a concentrated bulge with a fairly uniform falloff in intensity outwards. The core exhibits a yellowish-white color, suggesting a population of older stars, possibly with lower ongoing star formation. There's a slight indication of a flattened disk-like structure surrounding the central bulge, but it is mostly spheroidal. No significant dust lanes or spiral arms are visible, leading to the conclusion that it is in the later stages of galaxy evolution. There may be a slight disturbance in morphology but likely nothing significant. The galaxy appears fairly isolated, showing no strong signs of tidal interaction with neighboring galaxies, consistent with a relaxed morphology.
