The galaxy presents as a relatively small, disk-shaped structure. The central region exhibits a bright, compact core, possibly indicative of an active galactic nucleus or a dense stellar population. The disk component shows a color gradient, with bluer hues concentrated in a ring-like structure that is in the center of the galaxy, which may suggest regions of ongoing star formation. Fainter, redder colors are observed in the central disk, indicating older stellar populations or dust obscuration. The overall disk appears relatively smooth and featureless, with no prominent spiral arm structures or large-scale irregularities readily visible. A slight tidal distortion is observable in the bottom quadrant, with a hint of merging activity in the form of a faint tail extending outwards, though it is faint and more difficult to observe.
