The galaxy presents a predominantly smooth morphology, with a subtle suggestion of a disk-like structure. The light distribution exhibits a concentrated central region, likely indicating a bulge. The overall shape is somewhat elliptical, transitioning from round to slightly elongated. There are hints of minor disturbances in the galaxy's structure, but it is difficult to determine from this image whether they are due to a recent interaction. Given the luminosity, it is estimated that the stellar mass of the galaxy is quite large. Based on the low levels of recent star formation, it is likely a fairly inactive galaxy.
