The galaxy presents as a spiral galaxy with a moderately sized central bulge. The spiral arms appear to have a winding structure that is neither tightly wound nor loosely extended. The galaxy exhibits a two-arm spiral structure. The galaxy shows some indications of tidal disturbances, but not a full merger event. The central bulge appears yellowish, suggesting an older stellar population. The spiral arms show subtle variations in color, with some bluer regions potentially indicating ongoing star formation. The disc is not perfectly edge on, with a clear view of the spiral structure. The galaxy appears to be unbarred or only weakly barred. The galaxy exhibits a relatively high star formation rate.
