The galaxy presents as a diffuse, centrally concentrated object. The core region exhibits a yellow-orange hue, suggesting an older stellar population. Moving outwards from the core, there appears to be a gradual transition to a less defined disk or envelope. Faint blue regions are observed in this outer area, potentially indicative of some ongoing star formation, albeit at a low rate. The overall structure is relatively smooth, with no clear evidence of spiral arms or a prominent disk. There are slight irregularities within the outer region, but it's difficult to say definitively whether it's the result of a minor disturbance or a subtle morphological feature of the galaxy itself. The object appears relatively isolated with no clear signs of a major ongoing merger. The inferred mass of this system is substantial, suggesting it is a fairly large and gravitationally bound structure. Based on the color indices, star formation is weak overall.
