The galaxy presents as a spiral type, observed at a slight angle. It exhibits a moderately bright central bulge, appearing yellowish-white, suggesting an older stellar population concentrated at the core. The spiral arms are well-defined, displaying a somewhat patchy distribution of bluer light, indicative of ongoing star formation regions. The disk component appears relatively thin and elongated, suggesting the galaxy is significantly inclined relative to our line of sight, but not fully edge-on. The spiral arms are relatively tightly wound, but with medium definition. The spiral structure shows two prominent arms. There is no clear sign of a strong bar structure. Overall, the galaxy shows no evidence of recent major merger activity.
