The galaxy presents as a single, relatively smooth object with a concentrated central bulge. It appears elliptical in shape, with a high degree of symmetry. There is minimal evidence of spiral arm structure. The light distribution suggests a fairly uniform stellar population, with a color gradient from a yellowish-white core to a slightly redder halo. No significant dust lanes or other morphological disturbances are visible. The overall appearance is consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy at a moderate redshift. The galaxy does not show any signs of recent or ongoing major merging activity.
