The galaxy presents as a somewhat elliptical, centrally concentrated object. Its morphology appears to be largely smooth, with minimal discernible structure such as spiral arms or dust lanes. The galaxy exhibits a dominant yellowish hue, suggesting an older stellar population and potentially lower ongoing star formation. The object's light distribution gradually fades from the center, indicating a lack of distinct features or regions of intense star formation. There is no clear evidence of strong tidal interactions or recent merger events, although a slight asymmetry cannot be entirely ruled out.
