The target galaxy presents as an elongated structure, highly inclined with respect to our line of sight, indicating an edge-on or nearly edge-on orientation.  It exhibits a central bulge that appears moderately prominent and somewhat rounded. The disk component appears relatively smooth, lacking significant visible substructure such as prominent spiral arms. The galaxy's color suggests a population dominated by older stars, though some bluer regions may hint at ongoing star formation. There is no obvious indication of interaction or merging with another galaxy, although there may be minor disturbances.
