The observed galaxy presents as a primarily smooth object, exhibiting a relatively round morphology. The light distribution appears fairly uniform across the galaxy's body. A slight deviation from perfect circularity is present, but it is not significantly elongated. There is no obvious disk structure. No strong tidal features or indications of recent major merger activity are present, and no significant dust lanes are apparent. There may be a faint indication of a minor disturbance of the galaxy, however, this is indistinct and difficult to determine. The galaxy displays a moderate color gradient, trending toward bluer hues in the outer regions and redder tones towards the center.
