The galaxy presents as a relatively compact, luminous structure with a dominant yellowish-orange hue, suggesting an older stellar population. The light distribution is mostly smooth, with a central concentration of luminosity. There appears to be a slight elongation or distortion in its shape, perhaps indicating a minor interaction or internal disturbance. There may be some faint wisps or tidal features extending from the galaxy. The galaxy does not exhibit prominent spiral arms or a well-defined disk-like structure.
