The galaxy presents as a moderately luminous, elongated spheroid. The light distribution suggests a relatively smooth morphology, with a gradual increase in intensity toward the galactic center, indicating a high degree of central concentration. The galaxy exhibits an overall yellow-white hue, suggestive of a stellar population dominated by older, evolved stars. There is a slight asymmetry along the major axis, with a subtle extension or possible faint tidal feature, suggesting a potential interaction or past merger event, although no major disturbances are apparent within the main galactic body.
