The galaxy appears as a relatively compact object. Morphologically, it presents a smooth, somewhat amorphous structure, lacking a well-defined spiral arm pattern or a prominent bulge. There are no signs of a pronounced disk component. The galaxy exhibits a redder hue in the central region, transitioning to a bluer tint towards the outer edges. No obvious signs of tidal tails or other indicators of recent major mergers are apparent, although the possibility of minor disturbances cannot be ruled out at this resolution.
