The galaxy presents as a somewhat luminous, disk-shaped structure. Its color appears to be in the yellow-white spectrum, hinting at a potentially older stellar population. The morphology leans toward a relatively smooth overall appearance, although there may be some slight deviations from perfect symmetry, suggesting minor disturbances or internal structures. The ellipticity indicates a shape that is between circular and cigar shaped, but closer to circular. There is a smaller object located near it, that could potentially be causing a merger. If there is a merger, it is not a strong or intense merger and could be categorized as minor disturbance or an early stage of merging based on the images alone. Further spectral analysis would be needed to better determine the galaxy's composition, age, and dynamic state.