The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology with a high degree of roundness. A dominant, bright central bulge is observed. Moving outwards from the core, the color transitions smoothly into a redder hue, suggesting a population of older stars. The lack of distinct spiral arms, dust lanes, or pronounced features indicates a quiescent system with minimal ongoing star formation. There is also a slight possibility that this galaxy is undergoing a minor interaction or disturbance, but otherwise the galaxy appears to be isolated.
