The galaxy presents as a single, relatively smooth and centrally concentrated object. Its morphology appears largely elliptical, with a high degree of roundness observed in its overall shape. There's no discernible spiral structure or distinct features suggesting significant ongoing star formation, such as prominent HII regions. The light distribution is generally smooth and decreases gradually from the bright central region outwards. The color profile indicates an older stellar population, leaning towards redder hues. There is no evidence of significant tidal disturbances or ongoing merger activity, and no major distortions are visible in the galaxy's morphology. It does not appear to be a disk galaxy.
