The galaxy presents as a single, relatively smooth, and well-defined luminous object. Its overall shape appears approximately round. There is a slight color gradient visible, with the core exhibiting a brighter, more yellow-toned appearance, potentially indicative of an older stellar population. The outer regions of the galaxy display a subtle fading in intensity and a slight shift towards redder hues. No distinct spiral arms or bar structures are apparent. There is no indication of a major ongoing merger event; the galaxy appears relatively undisturbed. Minor irregularities or faint extensions are not visibly discernible in the galaxy's outer regions. Its morphological classification appears to be consistent with an elliptical galaxy, or potentially a lenticular galaxy viewed face-on.
