The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth morphology without apparent spiral arm structures or a distinct bar. Its shape appears generally elliptical, nearing a circular form. A slight color gradient is discernible, with the central region showing a more yellowish or golden hue, possibly indicating a higher concentration of older stellar populations. Moving outward, a subtle shift towards redder tones suggests a gradual change in stellar composition or dust content. There's no clear evidence of ongoing major mergers or significant tidal disturbances; however, there's a possibility of minor interactions. The galaxy’s overall appearance suggests a potentially evolved system with a relatively high degree of spheroidal component dominance and a moderate level of star formation.
