The galaxy presents a generally elliptical morphology, appearing relatively smooth with a bright central bulge. There is a hint of a disk, possibly with some disturbances. A brighter region exists that may indicate an active galactic nucleus. There appears to be suppressed star formation activity in the galaxy based on the coloring and general morphology. A tidal tail may also be present, which points to possible merging activity. The galaxy has a yellowish-red hue, which could indicate an older stellar population, a higher concentration of dust, or a higher redshift.
