The galaxy presents a generally smooth and elliptical morphology. It is characterized by a dominant central bulge, exhibiting a concentrated and luminous core. The color profile suggests a population of older stars, contributing to the galaxy's yellowish hue. There is no apparent disk structure or spiral arm features visible within the resolution of the image. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger activity or tidal distortions. There may be some very minor disturbances present.
