The galaxy exhibits a roughly elliptical morphology. Its core is bright and compact, displaying a saturated white hue, indicating a high concentration of stars and/or active galactic nucleus activity. The galaxy's light is dominated by shorter wavelengths, displaying a blue halo, which may indicate active star formation. The central region has a distinct turquoise color, perhaps a result of a combination of the blue halo and an underlying population of older stars, indicating it is no longer forming stars as actively as it used to. There are indications of potential tidal disturbances or faint plumes extending outwards, especially on the left side. These features might be indicative of a past or ongoing minor merger event.
