The galaxy presents as a relatively small, edge-on spiral system. It exhibits a flattened disk structure with minimal discernible bulge. The galaxy appears smooth, with no strong evidence of significant star formation regions or prominent dust lanes. Its color suggests a relatively evolved stellar population, potentially dominated by older, redder stars. There is no visible sign of interaction or merging activity. The object exhibits a consistent structure and color, hinting towards a relatively quiescent stage in its evolution.
