The galaxy presents as a centrally concentrated, relatively smooth object. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population and potentially low levels of active star formation. The outer regions of the galaxy appear less concentrated, displaying a fainter, greenish-blue tint, possibly suggesting the presence of some younger, hotter stars. While the object is largely smooth, a subtle asymmetry in the outer regions hints at a possible disk-like structure or a past minor interaction. No obvious spiral arms or strong tidal features are apparent. The galaxy appears somewhat elliptical in shape, but not highly elongated.
