The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The observed color is yellowish-orange, suggesting a stellar population dominated by older, cooler stars. The overall shape approximates a circular profile, with only minor deviations from perfect roundness. There are no readily discernible spiral arm structures or dust lanes. There is a nearby galaxy that is slightly smaller and less concentrated than the main galaxy. This system does not show any strong indication of tidal interactions or ongoing merging activity, though some minor disturbances cannot be ruled out.
