The galaxy appears as a small, faint red object. Its morphology is difficult to discern precisely due to its size and faintness. Based on the red color, the galaxy likely has a significant population of older stars, or a considerable amount of dust extinction. The light profile appears relatively smooth, but there might be some subtle, low-contrast features or irregularities present, perhaps suggesting a weak disk or disturbances. There may be subtle distortions or indications of past or ongoing interactions. At this resolution, determining if this is a spiral or elliptical galaxy is not possible. Higher resolution imaging or spectroscopic data would be valuable to determine the galaxy's type and characteristics.
