The galaxy presents as a smooth, centrally concentrated light distribution with a relatively round morphology. There is no discernible spiral structure or significant morphological disturbance evident. The galaxy exhibits a color gradient, with a more yellow-orange hue towards the core, suggesting an older stellar population dominating the central region. The outer regions appear slightly bluer, possibly indicative of more recent, albeit low, star formation activity. The overall appearance suggests an elliptical galaxy or a lenticular galaxy viewed face-on. The galaxy is estimated to be of moderate size for typical galaxies.
