The galaxy presents as a relatively luminous object with a centrally concentrated light profile. Morphologically, it appears to exhibit characteristics of both smooth and featured components, suggesting a complex structure. The overall shape is somewhat elliptical, with a noticeable elongation. There is a notable component which may be a disk. It appears the galaxy may be undergoing a merger, as there is a second distinct concentration of light that is separate from the main body, and the central morphology of the galaxy is disturbed. There may be a degree of tidal interaction. The color suggests the presence of both older stellar populations, implied by redder hues, and potentially ongoing or recent star formation activity, indicated by bluer colors and potentially indicating a spiral galaxy. The Sersic index suggest a late-type galaxy.
