The galaxy appears as a concentrated, moderately luminous object with a dominant yellowish-orange hue. The light profile seems relatively smooth, lacking any distinct spiral arm structures or prominent dust lanes in this image resolution. There is a subtle suggestion of elongation, but it is generally round. The color indicates an older stellar population and possibly lower ongoing star formation activity within the galaxy. There are slight, possibly tidal irregularities. This galaxy is not isolated; it appears to be part of a small system of interacting objects.