The galaxy presents as a concentrated central bulge with a surrounding, less defined disk. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The disk component appears less distinct, presenting a fainter blueish tint, which could indicate regions of more recent star formation. The overall shape leans towards elliptical. There are no obvious spiral arm structures or strong irregularities visible, and the galaxy seems relatively undisturbed.
