The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. It possesses a bright, yellowish core which likely indicates an older stellar population. The outer regions display a fainter, slightly bluer hue suggesting the presence of more recent star formation within the galaxy's disk. The overall shape leans more toward round rather than highly elongated. There appears to be no significant signs of major disturbances or ongoing merger activity, although there may be some signs of minor tidal activity.
