The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an approximately round morphology with a dominant yellowish hue in the central region, suggesting an older stellar population. There is an extension of diffuse light towards the left side, displaying a slightly bluer color, which could indicate the presence of younger stars or ongoing star formation in that region. A fainter, reddish component is seen towards the right, potentially caused by dust obscuration or a population of evolved red giant stars. Overall, the galaxy seems to be largely undisturbed, without prominent spiral arms or irregular features.
