The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is somewhat elongated, approaching a cigar-like appearance. A central bulge is evident, brighter and more condensed than the surrounding regions. The light distribution from the core outwards appears relatively uniform. The galaxy exhibits a blue hue, which could indicate ongoing, albeit subdued, star formation activity. There are no obvious spiral arm structures or significant dust lanes visible in this image, leading me to conclude that this is a galaxy with a dominant smooth component. There are hints of some disturbances in the outer edges of the disk, but no major mergers can be seen in this image.
