The galaxy presents as a roughly elliptical, spheroid-shaped object. Its core exhibits a concentrated, bright, yellow-orange hue, suggesting a population of older stars. The isophotes appear generally smooth, though with some indication of substructure or possible tidal disturbances on its periphery, suggesting a past or ongoing interaction. One area appears more disturbed than the rest, with a faint blue tinge to the outskirts on the right side, which may be suggestive of some level of recent or current star formation, possibly triggered by interaction with another galaxy or perhaps an inflow of gas. The galaxy's overall color suggests a lack of significant ongoing, widespread star formation, indicating it is a relatively passive system. There are also indications of a possible merger event taking place.
