This galaxy presents as a generally smooth object, with a concentrated central bulge or core region. The light distribution suggests a relatively uniform stellar population, with the brightest emissions concentrated towards the center, fading gradually outward. A distinct disk component or spiral arm structure is not readily apparent. The color profile indicates a redder hue, particularly in the central region. This suggests a population of older, cooler stars and/or significant dust obscuration. The overall morphology is consistent with an elliptical galaxy or possibly a lenticular galaxy seen at a relatively face-on angle. There is no strong evidence of ongoing major mergers or tidal disturbances. The circularity is high, indicating it is round. Minor asymmetries are present, potentially due to minor interactions or internal structures.
