The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form is somewhat elongated, but not highly so. The galaxy exhibits a diffuse blueish hue in its central region. This color suggests the presence of a moderate population of relatively young, hot stars, potentially indicative of ongoing star formation, although not at an extremely high rate. The outer regions of the galaxy become fainter and redder, transitioning gradually from the central region. There is no obvious spiral structure, bar, or strong tidal features visible. The morphology of the galaxy does not show any signs of a major merger, but there is possibly some very slight disturbance of the outer parts of the galaxy.
