The galaxy presents as a somewhat elongated structure, with a cigar-shaped appearance. It shows a smooth light distribution. There is little or no evidence of spiral arms or distinct features such as prominent dust lanes within the galaxy. The core exhibits a greater concentration of luminosity. The overall color profile suggests a population dominated by older stars and comparatively less on-going star formation activity. It is a moderately large galaxy. It is likely an elliptical galaxy. There is no strong evidence of a major ongoing merger.
