The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to be dominated by an elliptical distribution. There is a slight color gradient observed, where the central region appears more yellow, suggesting the presence of an older stellar population, while the outer regions show hints of blue, perhaps indicating some ongoing star formation. No prominent spiral arms or significant dust lanes are discernible. There are some irregular features which indicate possible tidal disturbances or a minor merger. The object exhibits a roughly round morphology.
