The galaxy presents as a faint, elongated structure with a roughly elliptical morphology. The central region exhibits a brighter, more concentrated luminosity profile, suggesting a possible bulge component. A faint disk may be present but this is uncertain due to the galaxy's inclination relative to our line of sight. Color gradients suggest the presence of ongoing or recent star formation. There are hints of some disturbances in the galaxy shape, possibly indicating tidal interactions or internal dynamical processes. The galaxy may be merging based on its shape, but the lack of clear secondary nuclei makes that uncertain. The color of the galaxy is relatively uniform, implying the stellar populations are of similar ages.
