The galaxy presents a somewhat elliptical morphology, though not perfectly spherical. The radial color profile suggests a central bulge dominated by older stellar populations, appearing yellowish-orange. The outer regions exhibit bluer hues, possibly indicative of more recent star formation. These regions appear less structured, displaying a somewhat irregular shape. There is marginal evidence for some mild disturbance in its morphology, possibly suggesting a past or ongoing minor interaction. Overall, the galaxy appears to be in a transitional phase between a purely elliptical and a more disk-dominated system.
