The galaxy presents as a spiral type, observed at a slight angle relative to edge-on. The central bulge exhibits a concentrated luminosity. The spiral arms appear prominent and well-defined, tracing a relatively tight winding pattern around the core. Two dominant spiral arms are visible. There is evidence of a bar-like structure extending through the center of the galaxy, although it does not appear highly pronounced. The color distribution suggests active star formation within the spiral arms. The overall morphology indicates a galaxy that is not currently undergoing a major merging event.
