The galaxy presents a generally smooth morphology, though there are subtle irregularities indicative of possible disturbances. The main body of the galaxy appears elongated, leaning towards a rounded shape, but not perfectly spherical. Within this, there may be a slight suggestion of a disk-like component, although it is not a prominent feature. Evidence of merging is subtle, but there are slight distortions that would suggest a minor disturbance or perhaps an ongoing minor merger. It is a fairly luminous galaxy, displaying a spectral energy distribution that exhibits an increased presence toward the redder bands. There are signs of star formation, but this is occurring at a slow rate.
