The observed galaxy appears as a luminous entity with a slightly irregular morphology. The light distribution suggests two distinct but connected components, potentially indicative of a merging system or a galaxy with a disturbed disk. The primary component exhibits a more diffuse and elongated appearance. The secondary component is smaller, brighter and more concentrated. The overall color is yellowish, suggesting a stellar population with a significant fraction of older stars. There are no clearly defined spiral arms or a prominent bulge visible, although the central region appears somewhat denser. The light appears relatively smooth, potentially indicating that this is a disk galaxy viewed at an angle, or an elliptical. The light intensity decreases gradually from the center outwards. There appears to be some indication of tidal features, suggesting potential ongoing gravitational interaction.
