The galaxy presents as a generally smooth, elliptical morphology, exhibiting a concentrated central bulge that appears yellowish-white in color. Moving outward from the core, a fainter, bluish halo is observed, suggesting a population of younger, bluer stars residing further from the galactic center. The overall shape tends towards spheroidal, with a slight elongation, but no discernible spiral arm structures or significant dust lanes are apparent within the resolution of the image. There are hints of possible minor tidal disturbances or faint plumes extending from the galaxy, which would suggest a past interaction with another galactic body, or possibly a merger. However, these features, if real, are extremely subtle and require further investigation. The lack of significant dust features coupled with the smooth morphology indicates that this is likely a galaxy that is past its peak star formation period, though the presence of some blue light indicates that star formation continues to occur at some level. 
