The galaxy presents as a somewhat elliptical object with a dominant central bulge. There's a suggestion of a disk-like structure surrounding the bulge, though it is not clearly defined, and is relatively smooth. The color gradient suggests a higher concentration of older stars towards the center, with a slightly bluer hue in the outer regions. There are no prominent spiral arms or significant dust lanes visible. There is some subtle distortion in the shape, potentially indicating a minor gravitational interaction or internal disturbance. The galaxy appears to be in a relatively quiescent state, with low levels of on-going star formation.
