The galaxy presents as a relatively smooth, centrally concentrated object with a round morphology. The core region appears to be composed of older stellar populations as indicated by the yellowish-white color. This transitions outward to a less concentrated disk with a faint bluish hue, potentially indicative of more recent star formation, although overall star formation appears to be low. There is no clear evidence of spiral arm structure or significant dust lanes. The general lack of significant distortions or irregularities suggests it is not currently undergoing a major merger event, though there may be evidence of minor tidal features upon further investigation. The object spans an approximate diameter of 10 kpc.
